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ALMA Lensing Cluster Survey: Full Spectral Energy Distribution Analysis of z ∼ 0.5–6 Lensed Galaxies Detected with millimeter Observations (2024)
Journal Article
Uematsu, R., Ueda, Y., Kohno, K., Toba, Y., Yamada, S., Smail, I., …Sun, F. (2024). ALMA Lensing Cluster Survey: Full Spectral Energy Distribution Analysis of z ∼ 0.5–6 Lensed Galaxies Detected with millimeter Observations. Astrophysical Journal, 965(2), Article 108. https://doi.org/10.3847/1538-4357/ad26f7

Sub/millimeter galaxies are a key population for the study of galaxy evolution because the majority of star formation at high redshifts occurred in galaxies deeply embedded in dust. To search for this population, we have performed an extensive survey... Read More about ALMA Lensing Cluster Survey: Full Spectral Energy Distribution Analysis of z ∼ 0.5–6 Lensed Galaxies Detected with millimeter Observations.

Obscured star formation in clusters at z = 1.6–2.0: massive galaxy formation and the reversal of the star formation–density relation (2024)
Journal Article
Smail, I. (2024). Obscured star formation in clusters at z = 1.6–2.0: massive galaxy formation and the reversal of the star formation–density relation. Monthly Notices of the Royal Astronomical Society, 529(3), 2290-2308. https://doi.org/10.1093/mnras/stae692

Clusters of galaxies at z   1 are expected to be increasingly active sites of star formation. To test this, an 850 m survey was undertaken of eight clusters at z = 1.6–2.0 using SCUBA-2 on the James Clerk Maxwell Telescope. Mid-infrared properties w... Read More about Obscured star formation in clusters at z = 1.6–2.0: massive galaxy formation and the reversal of the star formation–density relation.

An ALMA Spectroscopic Survey of the Brightest Submillimeter Galaxies in the SCUBA-2-COSMOS Field (AS2COSPEC): Physical Properties of z = 2–5 Ultra- and Hyperluminous Infrared Galaxies (2024)
Journal Article
Liao, C., Chen, C., Wang, W., Smail, I., Ao, Y., Chapman, S. C., …Zhao, Y. (2024). An ALMA Spectroscopic Survey of the Brightest Submillimeter Galaxies in the SCUBA-2-COSMOS Field (AS2COSPEC): Physical Properties of z = 2–5 Ultra- and Hyperluminous Infrared Galaxies. Astrophysical Journal, 961(2), Article 226. https://doi.org/10.3847/1538-4357/ad148c

We report the physical properties of the 18 brightest (S 870 μm = 12.4–19.2 mJy) and not strongly lensed 870 μm–selected dusty star-forming galaxies (DSFGs), also known as submillimeter galaxies (SMGs), in the COSMOS field. This sample is part of an... Read More about An ALMA Spectroscopic Survey of the Brightest Submillimeter Galaxies in the SCUBA-2-COSMOS Field (AS2COSPEC): Physical Properties of z = 2–5 Ultra- and Hyperluminous Infrared Galaxies.

PEARLS: Near-infrared Photometry in the JWST North Ecliptic Pole Time Domain Field * * Partly based on observations taken with the MMT, a joint facility operated by the University of Arizona and the Smithsonian Institution. (2023)
Journal Article
Willmer, C. N. A., Ly, C., Kikuta, S., Kattner, S. A., Jansen, R. A., Cohen, S. H., …Grogin, N. A. (2023). PEARLS: Near-infrared Photometry in the JWST North Ecliptic Pole Time Domain Field * * Partly based on observations taken with the MMT, a joint facility operated by the University of Arizona and the Smithsonian Institution. Astrophysical Journal Supplement, 269(1), Article 21. https://doi.org/10.3847/1538-4365/acf57d

We present near-infrared (NIR) ground-based Y, J, H, and K imaging obtained in the James Webb Space Telescope (JWST) North Ecliptic Pole Time Domain Field (NEP TDF) using the MMT-Magellan Infrared Imager and Spectrometer on the MMT. These new observa... Read More about PEARLS: Near-infrared Photometry in the JWST North Ecliptic Pole Time Domain Field * * Partly based on observations taken with the MMT, a joint facility operated by the University of Arizona and the Smithsonian Institution..

Hidden Giants in JWST's PEARLS: An Ultramassive z = 4.26 Submillimeter Galaxy that Is Invisible to HST (2023)
Journal Article
Smail, I., Dudzevičiūtė, U., Gurwell, M., Fazio, G. G., Willner, S. P., Swinbank, A. M., …Yun, M. (2023). Hidden Giants in JWST's PEARLS: An Ultramassive z = 4.26 Submillimeter Galaxy that Is Invisible to HST. Astrophysical Journal, 958(1), 36. https://doi.org/10.3847/1538-4357/acf931

We present a multiwavelength analysis using the Submillimeter Array (SMA), James Clerk Maxwell Telescope, NOEMA, JWST, the Hubble Space Telescope (HST), and the Spitzer Space Telescope of two dusty strongly star-forming galaxies, 850.1 and 850.2, see... Read More about Hidden Giants in JWST's PEARLS: An Ultramassive z = 4.26 Submillimeter Galaxy that Is Invisible to HST.

VLA Legacy Survey of Molecular Gas in Massive Star-forming Galaxies at High Redshift (2023)
Journal Article
Castillo, M. F., Hodge, J., Rybak, M., van der Werf, P., Smail, I., Birkin, J. E., …Dannerbauer, H. (2023). VLA Legacy Survey of Molecular Gas in Massive Star-forming Galaxies at High Redshift. Astrophysical Journal, 945(2), Article 128. https://doi.org/10.3847/1538-4357/acb931

We present the initial results of an ongoing survey with the Karl G. Jansky Very Large Array targeting the CO(J = 1–0) transition in a sample of 30 submillimeter-selected, dusty star-forming galaxies (SFGs) at z = 2–5 with existing mid-J CO detection... Read More about VLA Legacy Survey of Molecular Gas in Massive Star-forming Galaxies at High Redshift.

The JCMT SCUBA-2 Survey of the James Webb Space Telescope North Ecliptic Pole Time-Domain Field (2023)
Journal Article
Hyun, M., Im, M., Smail, I. R., Cotton, W. D., Birkin, J. E., Kikuta, S., …Yan, H. (2023). The JCMT SCUBA-2 Survey of the James Webb Space Telescope North Ecliptic Pole Time-Domain Field. Astrophysical Journal Supplement, 264(1), Article 19. https://doi.org/10.3847/1538-4365/ac9bf4

The James Webb Space Telescope Time-Domain Field (JWST-TDF) is an ∼14′ diameter field near the North Ecliptic Pole that will be targeted by one of the JWST Guaranteed Time Observations programs. Here, we describe our James Clerk Maxwell Telescope SCU... Read More about The JCMT SCUBA-2 Survey of the James Webb Space Telescope North Ecliptic Pole Time-Domain Field.

JWST’s PEARLS: A JWST/NIRCam View of ALMA Sources (2023)
Journal Article
Cheng, C., Huang, J., Smail, I., Yan, H., Cohen, S. H., Jansen, R. A., …Ryan, R. E. (2023). JWST’s PEARLS: A JWST/NIRCam View of ALMA Sources. Astrophysical Journal Letters, 942(1), Article L19. https://doi.org/10.3847/2041-8213/aca9d0

We report the results of James Webb Space Telescope/NIRCam observations of 19 (sub)millimeter sources detected by the Atacama Large Millimeter Array (ALMA). The accurate ALMA positions allowed unambiguous identifications of their NIRCam counterparts.... Read More about JWST’s PEARLS: A JWST/NIRCam View of ALMA Sources.

JWST PEARLS. Prime Extragalactic Areas for Reionization and Lensing Science: Project Overview and First Results (2022)
Journal Article
Windhorst, R. A., Cohen, S. H., Jansen, R. A., Summers, J., Tompkins, S., Conselice, C. J., …Zhao, X. (2023). JWST PEARLS. Prime Extragalactic Areas for Reionization and Lensing Science: Project Overview and First Results. Astronomical Journal, 165(1), Article 13. https://doi.org/10.3847/1538-3881/aca163

We give an overview and describe the rationale, methods, and first results from NIRCam images of the JWST “Prime Extragalactic Areas for Reionization and Lensing Science” (PEARLS) project. PEARLS uses up to eight NIRCam filters to survey several prim... Read More about JWST PEARLS. Prime Extragalactic Areas for Reionization and Lensing Science: Project Overview and First Results.

An Ultra-deep Multiband Very Large Array (VLA) Survey of the Faint Radio Sky (COSMOS-XS): New Constraints on the Cosmic Star Formation History (2022)
Journal Article
van der Vlugt, D., Hodge, J. A., Algera, H. S. B., Smail, I., Leslie, S. K., Radcliffe, J. F., …Röttgering, H. (2022). An Ultra-deep Multiband Very Large Array (VLA) Survey of the Faint Radio Sky (COSMOS-XS): New Constraints on the Cosmic Star Formation History. Astrophysical Journal, 941(1), Article 10. https://doi.org/10.3847/1538-4357/ac99db

We make use of ultra-deep 3 GHz Karl G. Jansky Very Large Array (VLA) observations of the COSMOS field from the multiband COSMOS-XS survey to infer radio luminosity functions (LFs) of star-forming galaxies (SFGs). Using ∼1300 SFGs with redshifts out... Read More about An Ultra-deep Multiband Very Large Array (VLA) Survey of the Faint Radio Sky (COSMOS-XS): New Constraints on the Cosmic Star Formation History.

ALMACAL IX: Multiband ALMA survey for dusty star-forming galaxies and the resolved fractions of the cosmic infrared background (2022)
Journal Article
Chen, J., Ivison, R., Zwaan, M. A., Smail, I., Klitsch, A., Péroux, C., …Lagos, C. (2023). ALMACAL IX: Multiband ALMA survey for dusty star-forming galaxies and the resolved fractions of the cosmic infrared background. Monthly Notices of the Royal Astronomical Society, 518(1), 1378-1397. https://doi.org/10.1093/mnras/stac2989

Wide, deep, blind continuum surveys at submillimetre/millimetre (submm/mm) wavelengths are required to provide a full inventory of the dusty, distant Universe. However, conducting such surveys to the necessary depth, with sub-arcsec angular resolutio... Read More about ALMACAL IX: Multiband ALMA survey for dusty star-forming galaxies and the resolved fractions of the cosmic infrared background.

ALMA Lensing Cluster Survey: ALMA-Herschel Joint Study of Lensed Dusty Star-forming Galaxies across z ≃ 0.5 – 6 (2022)
Journal Article
Sun, F., Egami, E., Fujimoto, S., Rawle, T., Bauer, F. E., Kohno, K., …Zitrin, A. (2022). ALMA Lensing Cluster Survey: ALMA-Herschel Joint Study of Lensed Dusty Star-forming Galaxies across z ≃ 0.5 – 6. Astrophysical Journal, 932(2), Article 77. https://doi.org/10.3847/1538-4357/ac6e3f

We present an ALMA-Herschel joint analysis of sources detected by the ALMA Lensing Cluster Survey (ALCS) at 1.15 mm. Herschel/PACS and SPIRE data at 100–500 μm are deblended for 180 ALMA sources in 33 lensing cluster fields that are detected either s... Read More about ALMA Lensing Cluster Survey: ALMA-Herschel Joint Study of Lensed Dusty Star-forming Galaxies across z ≃ 0.5 – 6.

An ALMA Spectroscopic Survey of the Brightest Submillimeter Galaxies in the SCUBA-2-COSMOS Field (AS2COSPEC): Survey Description and First Results (2022)
Journal Article
Chen, C., Liao, C., Smail, I., Swinbank, A., Ao, Y., Bunker, A., …Zhao, Y. (2022). An ALMA Spectroscopic Survey of the Brightest Submillimeter Galaxies in the SCUBA-2-COSMOS Field (AS2COSPEC): Survey Description and First Results. Astrophysical Journal, 929(2), Article 159. https://doi.org/10.3847/1538-4357/ac61df

We introduce an ALMA band 3 spectroscopic survey targeting the brightest submillimeter galaxies (SMGs) in the COSMOS field. Here we present the first results based on the 18 primary SMGs that have 870 μm flux densities of S870 = 12.4–19.3 mJy and are... Read More about An ALMA Spectroscopic Survey of the Brightest Submillimeter Galaxies in the SCUBA-2-COSMOS Field (AS2COSPEC): Survey Description and First Results.

COLDz: Probing Cosmic Star Formation With Radio Free–Free Emission (2022)
Journal Article
Algera, H. S., Hodge, J. A., Riechers, D. A., Leslie, S. K., Smail, I., Aravena, M., …Yun, M. (2022). COLDz: Probing Cosmic Star Formation With Radio Free–Free Emission. Astrophysical Journal, 924(2), https://doi.org/10.3847/1538-4357/ac34f5

Radio free–free emission is considered to be one of the most reliable tracers of star formation in galaxies. However, as it constitutes the faintest part of the radio spectrum—being roughly an order of magnitude less luminous than radio synchrotron e... Read More about COLDz: Probing Cosmic Star Formation With Radio Free–Free Emission.

Extensive Lensing Survey of Optical and Near-infrared Dark Objects (El Sonido): HST H-faint Galaxies behind 101 Lensing Clusters (2021)
Journal Article
Sun, F., Egami, E., Pérez-González, P. G., Smail, I., Caputi, K. I., Bauer, F. E., …Weaver, J. R. (2021). Extensive Lensing Survey of Optical and Near-infrared Dark Objects (El Sonido): HST H-faint Galaxies behind 101 Lensing Clusters. Astrophysical Journal, 922(2), https://doi.org/10.3847/1538-4357/ac2578

We present a Spitzer/IRAC survey of H-faint (H160 ≳ 26.4, < 5σ) sources in 101 lensing cluster fields. Across a CANDELS/Wide-like survey area of ∼648 arcmin2 (effectively ∼221 arcmin2 in the source plane), we have securely discovered 53 sources in th... Read More about Extensive Lensing Survey of Optical and Near-infrared Dark Objects (El Sonido): HST H-faint Galaxies behind 101 Lensing Clusters.

An extreme case of galaxy and cluster co-evolution at z  = 0.7 (2021)
Journal Article
Ebeling, H., Richard, J., Smail, I., Edge, A., Koekemoer, A., & Zalesky, L. (2021). An extreme case of galaxy and cluster co-evolution at z  = 0.7. Monthly Notices of the Royal Astronomical Society, 508(3), 3663-3671. https://doi.org/10.1093/mnras/stab2725

We report the discovery of eMACS J0252.4−2100 (eMACS J0252), a massive and highly evolved galaxy cluster at z = 0.703. Our analysis of Hubble Space Telescope imaging and VLT/MUSE and Keck/DEIMOS spectroscopy of the system finds a high-velocity disper... Read More about An extreme case of galaxy and cluster co-evolution at z  = 0.7.

Measurements of the Dust Properties in z ≃ 1–3 Submillimeter Galaxies with ALMA (2021)
Journal Article
da Cunha, E., Hodge, J., Casey, C., Algera, H., Kaasinen, M., Smail, I., …Zavala, J. (2021). Measurements of the Dust Properties in z ≃ 1–3 Submillimeter Galaxies with ALMA. Astrophysical Journal, 919(1), Article 30. https://doi.org/10.3847/1538-4357/ac0ae0

We present Atacama Large Millimeter/submillimeter Array (ALMA) 2 mm continuum observations of a complete and unbiased sample of 99 870 μm selected submillimeter galaxies (SMGs) in the Extended Chandra Deep Field South (ALESS). Our observations of eac... Read More about Measurements of the Dust Properties in z ≃ 1–3 Submillimeter Galaxies with ALMA.

ALMA Observations of Lyα Blob 1: Multiple Major Mergers and Widely Distributed Interstellar Media (2021)
Journal Article
Umehata, H., Smail, I., Steidel, C. C., Hayes, M., Scott, D., Swinbank, A., …Geach, J. (2021). ALMA Observations of Lyα Blob 1: Multiple Major Mergers and Widely Distributed Interstellar Media. Astrophysical Journal, 918(2), Article 69. https://doi.org/10.3847/1538-4357/ac1106

We present observations of a giant Lyα blob (LAB) in the SSA22 protocluster at z = 3.1, SSA22-LAB1, taken with the Atacama Large Millimeter/submillimeter Array. Dust continuum, along with [C ii] 158 μm and CO(4–3) line emission have been detected in... Read More about ALMA Observations of Lyα Blob 1: Multiple Major Mergers and Widely Distributed Interstellar Media.

Radio spectral properties of star-forming galaxies in the MIGHTEE-COSMOS field and their impact on the far-infrared-radio correlation (2021)
Journal Article
An, F., Vaccari, M., Smail, I., Jarvis, M., Whittam, I., Hale, C., …Randriamanakoto, Z. (2021). Radio spectral properties of star-forming galaxies in the MIGHTEE-COSMOS field and their impact on the far-infrared-radio correlation. Monthly Notices of the Royal Astronomical Society, 507(2), 2643-2658. https://doi.org/10.1093/mnras/stab2290

We study the radio spectral properties of 2094 star-forming galaxies (SFGs) by combining our early science data from the MeerKAT International GHz Tiered Extragalactic Exploration (MIGHTEE) survey with VLA, GMRT radio data, and rich ancillary data in... Read More about Radio spectral properties of star-forming galaxies in the MIGHTEE-COSMOS field and their impact on the far-infrared-radio correlation.

The KMOS galaxy evolution survey (KGES): the angular momentum of star-forming galaxies over the last ≍10 Gyr (2021)
Journal Article
Tiley, A. L., Gillman, S., Cortese, L., Swinbank, A., Dudzevičiūtė, U., Harrison, C., …Puglisi, A. (2021). The KMOS galaxy evolution survey (KGES): the angular momentum of star-forming galaxies over the last ≍10 Gyr. Monthly Notices of the Royal Astronomical Society, 506(1), 323-342. https://doi.org/10.1093/mnras/stab1692

We present the KMOS Galaxy Evolution Survey (KGES), a K-band Multi-Object Spectrograph (KMOS) study of the H α and [N II] emission from 288 K-band-selected galaxies at 1.2 ≲ z ≲ 1.8, with stellar masses in the range log10(M∗/M⊙)≈9 – 11.5. In this pap... Read More about The KMOS galaxy evolution survey (KGES): the angular momentum of star-forming galaxies over the last ≍10 Gyr.

ALMA Lensing Cluster Survey: Bright [C ii] 158 μm Lines from a Multiply Imaged Sub-L⋆ Galaxy at z = 6.0719 (2021)
Journal Article
Fujimoto, S., Oguri, M., Brammer, G., Yoshimura, Y., Laporte, N., González-López, J., …Espada, D. (2021). ALMA Lensing Cluster Survey: Bright [C ii] 158 μm Lines from a Multiply Imaged Sub-L⋆ Galaxy at z = 6.0719. Astrophysical Journal, 911(2), https://doi.org/10.3847/1538-4357/abd7ec

We present bright [C ii] 158 μm line detections from a strongly magnified and multiply imaged (μ ∼ 20–160) sub–L* (${M}_{\mathrm{UV}}=-{19.75}_{-0.44}^{+0.55}$) Lyman-break galaxy (LBG) at z = 6.0719 ± 0.0004, drawn from the ALMA Lensing Cluster Surv... Read More about ALMA Lensing Cluster Survey: Bright [C ii] 158 μm Lines from a Multiply Imaged Sub-L⋆ Galaxy at z = 6.0719.

The VLA Frontier Fields Survey: Deep, High-resolution Radio Imaging of the MACS Lensing Clusters at 3 and 6 GHz (2021)
Journal Article
Heywood, I., Murphy, E., Jiménez-Andrade, E., Armus, L., Cotton, W., DeCoursey, C., …Smirnov, O. (2021). The VLA Frontier Fields Survey: Deep, High-resolution Radio Imaging of the MACS Lensing Clusters at 3 and 6 GHz. Astronomical Journal, 910(2), Article 105. https://doi.org/10.3847/1538-4357/abdf61

The Frontier Fields project is an observational campaign targeting six galaxy clusters, with the intention of using the magnification provided by gravitational lensing to study galaxies that are extremely faint or distant. We used the Karl G. Jansky... Read More about The VLA Frontier Fields Survey: Deep, High-resolution Radio Imaging of the MACS Lensing Clusters at 3 and 6 GHz.

The VLA Frontier Field Survey: A Comparison of the Radio and UV/Optical Size of 0.3 ≲ z ≲ 3 Star-forming Galaxies (2021)
Journal Article
Jiménez-Andrade, E., Murphy, E., Heywood, I., Smail, I., Penner, K., Momjian, E., …Lazio, T. (2021). The VLA Frontier Field Survey: A Comparison of the Radio and UV/Optical Size of 0.3 ≲ z ≲ 3 Star-forming Galaxies. Astrophysical Journal, 910(2), Article 106. https://doi.org/10.3847/1538-4357/abe876

o investigate the growth history of galaxies, we measure the rest-frame radio, ultraviolet (UV), and optical sizes of 98 radio-selected, star-forming galaxies (SFGs) distributed over 0.3 ≲ z ≲ 3 with a median stellar mass of $\mathrm{log}({M}_{\star... Read More about The VLA Frontier Field Survey: A Comparison of the Radio and UV/Optical Size of 0.3 ≲ z ≲ 3 Star-forming Galaxies.

An ALMA/NOEMA survey of the molecular gas properties of high-redshift star-forming galaxies (2021)
Journal Article
Birkin, J. E., Weiss, A., Wardlow, J., Smail, I., Swinbank, A., Dudzevičiūtė, U., …van der Werf, P. (2021). An ALMA/NOEMA survey of the molecular gas properties of high-redshift star-forming galaxies. Monthly Notices of the Royal Astronomical Society, 501(3), 3926-3950. https://doi.org/10.1093/mnras/staa3862

We have used ALMA and NOEMA to study the molecular gas reservoirs in 61 ALMA-identified submillimetre galaxies (SMGs) in the COSMOS, UDS, and ECDFS fields. We detect 12CO (⁠Jup= 2–5) emission lines in 50 sources, and [C I](3P1 − 3P0) emission in eigh... Read More about An ALMA/NOEMA survey of the molecular gas properties of high-redshift star-forming galaxies.

An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: halo masses for submillimetre galaxies (2021)
Journal Article
Stach, S., Smail, I., Amvrosiadis, A., Swinbank, A., Dudzevičiūtė, U., Geach, J., …Wardlow, J. (2021). An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: halo masses for submillimetre galaxies. Monthly Notices of the Royal Astronomical Society, 504(1), https://doi.org/10.1093/mnras/stab714

We present an analysis of the spatial clustering of a large sample of high-resolution, interferometically identified, submillimetre galaxies (SMGs). We measure the projected cross-correlation function of ∼350 SMGs in the UKIDSS Ultra Deep-Survey Fiel... Read More about An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: halo masses for submillimetre galaxies.

ALMA 1.3 mm Survey of Lensed Submillimeter Galaxies Selected by Herschel: Discovery of Spatially Extended SMGs and Implications (2021)
Journal Article
Sun, F., Egami, E., Rawle, T. D., Walth, G. L., Smail, I., Dessauges-Zavadsky, M., …Valtchanov, I. (2021). ALMA 1.3 mm Survey of Lensed Submillimeter Galaxies Selected by Herschel: Discovery of Spatially Extended SMGs and Implications. Astrophysical Journal, 908(2), Article 192. https://doi.org/10.3847/1538-4357/abd6e4

We present an ALMA 1.3 mm (Band 6) continuum survey of lensed submillimeter galaxies (SMGs) at z = 1.0 to ∼3.2 with an angular resolution of ∼0farcs2. These galaxies were uncovered by the Herschel Lensing Survey and feature exceptionally bright far-i... Read More about ALMA 1.3 mm Survey of Lensed Submillimeter Galaxies Selected by Herschel: Discovery of Spatially Extended SMGs and Implications.

Resolving a dusty, star-forming SHiZELS galaxy at z = 2.2 with HST, ALMA, and SINFONI on kiloparsec scales (2021)
Journal Article
Cochrane, R., Best, P., Smail, I., Ibar, E., Cheng, C., Swinbank, A., …Dudzevi\vci\=ut\.e, U. (2021). Resolving a dusty, star-forming SHiZELS galaxy at z = 2.2 with HST, ALMA, and SINFONI on kiloparsec scales. Monthly Notices of the Royal Astronomical Society, 503(2), 2622-2638. https://doi.org/10.1093/mnras/stab467

We present ∼0.15 arcsec spatial resolution imaging of SHiZELS-14, a massive (⁠M∗∼1011M⊙⁠), dusty, star-forming galaxy at z = 2.24. Our rest-frame ∼1kpc-scale, matched-resolution data comprise four different widely used tracers of star formation: the... Read More about Resolving a dusty, star-forming SHiZELS galaxy at z = 2.2 with HST, ALMA, and SINFONI on kiloparsec scales.

Dust, Gas, and Metal Content in Star-forming Galaxies at z ∼ 3.3 Revealed with ALMA and Near-IR Spectroscopy (2021)
Journal Article
Suzuki, T. L., Onodera, M., Kodama, T., Daddi, E., Hayashi, M., Koyama, Y., …Tanaka, I. (2021). Dust, Gas, and Metal Content in Star-forming Galaxies at z ∼ 3.3 Revealed with ALMA and Near-IR Spectroscopy. Astrophysical Journal, 908(1), https://doi.org/10.3847/1538-4357/abd4e7

We conducted submillimeter observations with the Atacama Large Millimeter/submillimeter Array (ALMA) of star-forming galaxies at z ∼ 3.3, whose gas-phase metallicities have been measured previously. We investigated the dust and gas contents of the ga... Read More about Dust, Gas, and Metal Content in Star-forming Galaxies at z ∼ 3.3 Revealed with ALMA and Near-IR Spectroscopy.

FIR-luminous [C II] Emitters in the ALMA-SCUBA-2 COSMOS Survey (AS2COSMOS): The Nature of Submillimeter Galaxies in a 10 Comoving Megaparsec-scale Structure at z \ensuremath\sim 4.6 (2021)
Journal Article
Mitsuhashi, I., Matsuda, Y., Smail, I., Hayatsu, N., Simpson, J., Swinbank, A., …Sakamoto, S. (2021). FIR-luminous [C II] Emitters in the ALMA-SCUBA-2 COSMOS Survey (AS2COSMOS): The Nature of Submillimeter Galaxies in a 10 Comoving Megaparsec-scale Structure at z \ensuremath\sim 4.6. Astrophysical Journal, 907(2), Article 122. https://doi.org/10.3847/1538-4357/abcc72

We report the discovery of a 10 comoving megaparsec (cMpc)-scale structure traced by massive submillimeter galaxies (SMGs) at z ∼ 4.6. These galaxies are selected from an emission line search of ALMA Band 7 observations targeting 184 luminous submill... Read More about FIR-luminous [C II] Emitters in the ALMA-SCUBA-2 COSMOS Survey (AS2COSMOS): The Nature of Submillimeter Galaxies in a 10 Comoving Megaparsec-scale Structure at z \ensuremath\sim 4.6.

An ALMA survey of the S2CLS UDS field: optically invisible submillimetre galaxies (2021)
Journal Article
Smail, I., Dudzevičiūtė, U., Stach, S., Almaini, O., Birkin, J., Chapman, S., …van der Werf, P. (2021). An ALMA survey of the S2CLS UDS field: optically invisible submillimetre galaxies. Monthly Notices of the Royal Astronomical Society, 502(3), 3426-3435. https://doi.org/10.1093/mnras/stab283

We analyse a robust sample of 30 near-infrared-faint (KAB > 25.3, 5σ) submillimetre galaxies (SMGs) selected from a 0.96 deg2 field to investigate their properties and the cause of their faintness in optical/near-infrared wavebands. Our analysis expl... Read More about An ALMA survey of the S2CLS UDS field: optically invisible submillimetre galaxies.

An ALMA Survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS Field: The Far-infrared/Radio Correlation for High-redshift Dusty Star-forming Galaxies (2020)
Journal Article
Algera, H., Smail, I., Dudzevičiūtė, U., Swinbank, A., Stach, S., Hodge, J., …van der Werf, P. (2020). An ALMA Survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS Field: The Far-infrared/Radio Correlation for High-redshift Dusty Star-forming Galaxies. Astrophysical Journal, 903(2), Article 138. https://doi.org/10.3847/1538-4357/abb77b

We study the radio properties of 706 submillimeter galaxies (SMGs) selected at 870 μm with the Atacama Large Millimeter Array from the SCUBA-2 Cosmology Legacy Survey map of the Ultra Deep Survey field. We detect 273 SMGs at >4σ in deep Karl G. Jansk... Read More about An ALMA Survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS Field: The Far-infrared/Radio Correlation for High-redshift Dusty Star-forming Galaxies.

A Multiwavelength Analysis of the Faint Radio Sky (COSMOS-XS): the Nature of the Ultra-faint Radio Population (2020)
Journal Article
Algera, H., van der Vlugt, D., Hodge, J., Smail, I., Novak, M., Radcliffe, J., …Walter, F. (2020). A Multiwavelength Analysis of the Faint Radio Sky (COSMOS-XS): the Nature of the Ultra-faint Radio Population. Astrophysical Journal, 903(2), Article 139. https://doi.org/10.3847/1538-4357/abb77a

Ultra-deep radio surveys are an invaluable probe of dust-obscured star formation, but require a clear understanding of the relative contribution from radio active galactic nuclei (AGNs) to be used to their fullest potential. We study the composition... Read More about A Multiwavelength Analysis of the Faint Radio Sky (COSMOS-XS): the Nature of the Ultra-faint Radio Population.

The evolution of gas-phase metallicity and resolved abundances in star-forming galaxies at z ≍ 0.6-1.8 (2020)
Journal Article
Gillman, S., Tiley, A., Swinbank, A., Dudzevičiūtė, U., Sharples, R., Smail, I., …Stott, J. P. (2021). The evolution of gas-phase metallicity and resolved abundances in star-forming galaxies at z ≍ 0.6-1.8. Monthly Notices of the Royal Astronomical Society, 500(3), 4229-4247. https://doi.org/10.1093/mnras/staa3400

We present an analysis of the chemical abundance properties of ≈650 star-forming galaxies at z ≈ 0.6–1.8. Using integral-field observations from the K-band multi-object spectrograph (KMOS), we quantify the [N II]/H α emission-line ratio, a proxy for... Read More about The evolution of gas-phase metallicity and resolved abundances in star-forming galaxies at z ≍ 0.6-1.8.

Tracing the evolution of dust-obscured activity using sub-millimetre galaxy populations from STUDIES and AS2UDS (2020)
Journal Article
Dudzevičiūtė, U., Smail, I., Swinbank, A., Lim, C., Wang, W., Simpson, J., …Toba, Y. (2021). Tracing the evolution of dust-obscured activity using sub-millimetre galaxy populations from STUDIES and AS2UDS. Monthly Notices of the Royal Astronomical Society, 500(1), 942-961. https://doi.org/10.1093/mnras/staa3285

We analyse the physical properties of 121 SNR ≥ 5 sub-millimetre galaxies (SMGs) from the STUDIES 450 μm survey. We model their UV-to-radio spectral energy distributions using MAGPHYS+photo-z and compare the results to similar modelling of 850 μm-sel... Read More about Tracing the evolution of dust-obscured activity using sub-millimetre galaxy populations from STUDIES and AS2UDS.

The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: CO Excitation and Atomic Carbon in Star-forming Galaxies at z = 1–3 (2020)
Journal Article
Boogaard, L. A., Werf, P. V. D., Weiss, A., Popping, G., Decarli, R., Walter, F., …Wagg, J. (2020). The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: CO Excitation and Atomic Carbon in Star-forming Galaxies at z = 1–3. Astrophysical Journal, 902(2), Article 109. https://doi.org/10.3847/1538-4357/abb82f

We investigate the CO excitation and interstellar medium (ISM) conditions in a cold gas mass-selected sample of 22 star-forming galaxies at z = 0.46–3.60, observed as part of the ALMA Spectroscopic Survey in the Hubble Ultra Deep Field (ASPECS). Comb... Read More about The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: CO Excitation and Atomic Carbon in Star-forming Galaxies at z = 1–3.

The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Multiband Constraints on Line-luminosity Functions and the Cosmic Density of Molecular Gas (2020)
Journal Article
Decarli, R., Aravena, M., Boogaard, L., Carilli, C., González-López, J., Walter, F., …Weiss, A. (2020). The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Multiband Constraints on Line-luminosity Functions and the Cosmic Density of Molecular Gas. Astrophysical Journal, 902(2), Article 110. https://doi.org/10.3847/1538-4357/abaa3b

We present a CO and atomic fine-structure line-luminosity function analysis using the ALMA Spectroscopic Survey (ASPECS) in the Hubble Ultra Deep Field. ASPECS consists of two spatially overlapping mosaics that cover the entire ALMA 3 mm and 1.2 mm b... Read More about The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Multiband Constraints on Line-luminosity Functions and the Cosmic Density of Molecular Gas.

The ALMA Spectroscopic Survey Large Program: The Infrared Excess of z = 1.5–10 UV-selected Galaxies and the Implied High-redshift Star Formation History (2020)
Journal Article
Bouwens, R., González-López, J., Aravena, M., Decarli, R., Novak, M., Stefanon, M., …Wagg, J. (2020). The ALMA Spectroscopic Survey Large Program: The Infrared Excess of z = 1.5–10 UV-selected Galaxies and the Implied High-redshift Star Formation History. Astrophysical Journal, 902(2), Article 112. https://doi.org/10.3847/1538-4357/abb830

We make use of sensitive (9.3 μJy beam−1 rms) 1.2 mm continuum observations from the Atacama Large Millimeter/submillimeter Array (ALMA) Spectroscopic Survey in the Hubble Ultra-Deep Field (ASPECS) large program to probe dust-enshrouded star formatio... Read More about The ALMA Spectroscopic Survey Large Program: The Infrared Excess of z = 1.5–10 UV-selected Galaxies and the Implied High-redshift Star Formation History.

A kpc-scale-resolved study of unobscured and obscured star formation activity in normal galaxies at z = 1.5 and 2.2 from ALMA and HiZELS (2020)
Journal Article
Cheng, C., Ibar, E., Smail, I., Molina, J., Sobral, D., Escala, A., …Cirasuolo, M. (2020). A kpc-scale-resolved study of unobscured and obscured star formation activity in normal galaxies at z = 1.5 and 2.2 from ALMA and HiZELS. Monthly Notices of the Royal Astronomical Society, 499(4), 5241-5256. https://doi.org/10.1093/mnras/staa3036

We present Atacama Large Millimeter/Submillimeter Array (ALMA) continuum observations of a sample of nine star-forming galaxies at redshifts 1.47 and 2.23 selected from the High-z Emission Line Survey (HiZELS). Four galaxies in our sample are detecte... Read More about A kpc-scale-resolved study of unobscured and obscured star formation activity in normal galaxies at z = 1.5 and 2.2 from ALMA and HiZELS.

The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The Nature of the Faintest Dusty Star-forming Galaxies (2020)
Journal Article
Aravena, M., Boogaard, L., Gónzalez-López, J., Decarli, R., Walter, F., Carilli, C. L., …Wagg, J. (2020). The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The Nature of the Faintest Dusty Star-forming Galaxies. Astrophysical Journal, 901(1), Article 79. https://doi.org/10.3847/1538-4357/ab99a2

We present a characterization of the physical properties of a sample of 35 securely detected, dusty galaxies in the deep ALMA 1.2 mm image obtained as part of the ALMA Spectroscopic Survey in the Hubble Ultra Deep Field (ASPECS) Large Program. This s... Read More about The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The Nature of the Faintest Dusty Star-forming Galaxies.

The Evolution of the Baryons Associated with Galaxies Averaged over Cosmic Time and Space (2020)
Journal Article
Walter, F., Carilli, C., Neeleman, M., Decarli, R., Popping, G., Somerville, R. S., …Yung, L. A. (2020). The Evolution of the Baryons Associated with Galaxies Averaged over Cosmic Time and Space. Astrophysical Journal, 902(2), Article 111. https://doi.org/10.3847/1538-4357/abb82e

We combine the recent determination of the evolution of the cosmic density of molecular gas (H2) using deep, volumetric surveys, with previous estimates of the cosmic density of stellar mass, star formation rate and atomic gas (H i), to constrain the... Read More about The Evolution of the Baryons Associated with Galaxies Averaged over Cosmic Time and Space.

A Comparison of the Stellar, CO, and Dust-continuum Emission from Three Star-forming HUDF Galaxies at z ∼ 2 (2020)
Journal Article
Kaasinen, M., Walter, F., Novak, M., Neeleman, M., Smail, I., Boogaard, L., …Cox, P. (2020). A Comparison of the Stellar, CO, and Dust-continuum Emission from Three Star-forming HUDF Galaxies at z ∼ 2. Astrophysical Journal, 899(1), Article 37. https://doi.org/10.3847/1538-4357/aba438

We compare the extent of the dust, molecular gas, and stars in three star-forming galaxies, at z = 1.4, 1.6, and 2.7, selected from the Hubble Ultra Deep Field based on their bright carbon monoxide (CO) and dust-continuum emission as well as their la... Read More about A Comparison of the Stellar, CO, and Dust-continuum Emission from Three Star-forming HUDF Galaxies at z ∼ 2.

ALMA Deep Field in SSA22 (2020)
Journal Article
Umehata, H., Smail, I., Swinbank, A., Kohno, K., Tamura, Y., Wang, T., …Hayatsu, N. N. (2020). ALMA Deep Field in SSA22. Astronomy & Astrophysics, 640, Article L8. https://doi.org/10.1051/0004-6361/202038146

Deep surveys with the Atacama Large Millimeter Array (ALMA) have uncovered a population of dusty star-forming galaxies which are faint or even undetected at optical to near-infrared wavelengths. Their faintness at short wavelengths makes the detailed... Read More about ALMA Deep Field in SSA22.

The ALMA Spectroscopic Survey in the HUDF: Deep 1.2 mm Continuum Number Counts (2020)
Journal Article
González-López, J., Novak, M., Decarli, R., Walter, F., Aravena, M., Carilli, C., …Wagg, J. (2020). The ALMA Spectroscopic Survey in the HUDF: Deep 1.2 mm Continuum Number Counts. Astrophysical Journal, 897(1), Article 897. https://doi.org/10.3847/1538-4357/ab765b

We present the results from the 1.2 mm continuum image obtained as part of the Atacama Large Millimeter/ submillimeter Array Spectroscopic Survey in the Hubble Ultra Deep Field. The 1.2 mm continuum image has a size of 2.9 (4.2) arcmin2 within a prim... Read More about The ALMA Spectroscopic Survey in the HUDF: Deep 1.2 mm Continuum Number Counts.

Searching for obscured AGN in z ∼ 2 submillimetre galaxies (2020)
Journal Article
Chen, H., Garrett, M., Chi, S., Thomson, A., Barthel, P., Alexander, D., …Argo, M. (2020). Searching for obscured AGN in z ∼ 2 submillimetre galaxies. Astronomy & Astrophysics, 638, Article A113. https://doi.org/10.1051/0004-6361/201937162

Aims. Submillimetre-selected galaxies (SMGs) at high redshift (z ∼ 2) are potential host galaxies of active galactic nuclei (AGN). If the local Universe is a good guide, ∼50% of the obscured AGN amongst the SMG population could be missed even in the... Read More about Searching for obscured AGN in z ∼ 2 submillimetre galaxies.

VLA–ALMA Spectroscopic Survey in the Hubble Ultra Deep Field (VLASPECS): Total Cold Gas Masses and CO Line Ratios for z = 2–3 Main-sequence Galaxies (2020)
Journal Article
Riechers, D. A., Boogaard, L. A., Decarli, R., González-López, J., Smail, I., Walter, F., …van der Werf, P. (2020). VLA–ALMA Spectroscopic Survey in the Hubble Ultra Deep Field (VLASPECS): Total Cold Gas Masses and CO Line Ratios for z = 2–3 Main-sequence Galaxies. Astrophysical Journal Letters, 896(2), Article L21. https://doi.org/10.3847/2041-8213/ab9595

Using the NSF's Karl G. Jansky Very Large Array (VLA), we report six detections of CO(J = 1 → 0) emission and one upper limit in z = 2–3 galaxies originally detected in higher-J CO emission in the Atacama Large Millimeter/submillimeter Array Spectros... Read More about VLA–ALMA Spectroscopic Survey in the Hubble Ultra Deep Field (VLASPECS): Total Cold Gas Masses and CO Line Ratios for z = 2–3 Main-sequence Galaxies.

SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES). IV. Spatial Clustering and Halo Masses of Submillimeter Galaxies (2020)
Journal Article
Lim, C., Chen, C., Smail, I., Wang, W., Tee, W., Lin, Y., …Simpson, J. M. (2020). SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES). IV. Spatial Clustering and Halo Masses of Submillimeter Galaxies. Astrophysical Journal, 895(2), Article 104. https://doi.org/10.3847/1538-4357/ab8eaf

We analyze an extremely deep 450 μm image (1σ = 0.56 mJy beam−1 ) of a ;300 arcmin2 area in the CANDELS/ COSMOS field as part of the Sub-millimeter Common User Bolometric Array-2 Ultra Deep Imaging EAO Survey. We select a robust (signal-to-noise rati... Read More about SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES). IV. Spatial Clustering and Halo Masses of Submillimeter Galaxies.

COLDz: A High Space Density of Massive Dusty Starburst Galaxies ∼1 Billion Years after the Big Bang (2020)
Journal Article
Riechers, D. A., Hodge, J. A., Pavesi, R., Daddi, E., Decarli, R., Ivison, R. J., …Wagg, J. (2020). COLDz: A High Space Density of Massive Dusty Starburst Galaxies ∼1 Billion Years after the Big Bang. Astrophysical Journal, 895(2), Article 81. https://doi.org/10.3847/1538-4357/ab8c48

We report the detection of CO(J = 2 → 1) emission from three massive dusty starburst galaxies at z > 5 through molecular line scans in the NSF's Karl G. Jansky Very Large Array (VLA) CO Luminosity Density at High Redshift (COLDz) survey. Redshifts fo... Read More about COLDz: A High Space Density of Massive Dusty Starburst Galaxies ∼1 Billion Years after the Big Bang.

An ALMA survey of the brightest sub-millimetre sources in the SCUBA-2–COSMOS field (2020)
Journal Article
Simpson, J., Smail, I., Dudzevičiūtė, U., Matsuda, Y., Hsieh, B., Wang, W., …Zhao, Y. (2020). An ALMA survey of the brightest sub-millimetre sources in the SCUBA-2–COSMOS field. Monthly Notices of the Royal Astronomical Society, 495(3), 3409-3430. https://doi.org/10.1093/mnras/staa1345

We present an ALMA study of the ∼ 180 brightest sources in the SCUBA-2 850-μm map of the COSMOS field from the S2COSMOS survey, as a pilot study for AS2COSMOS – a full survey of the ∼ 1,000 sources in this field. In this pilot we have obtained 870-μm... Read More about An ALMA survey of the brightest sub-millimetre sources in the SCUBA-2–COSMOS field.

ALMACAL VII: First Interferometric Number Counts at 650 μm (2020)
Journal Article
Klitsch, A., Zwaan, M., Smail, I., Péroux, C., Biggs, A., Chen, C., …Dutta, R. (2020). ALMACAL VII: First Interferometric Number Counts at 650 μm. Monthly Notices of the Royal Astronomical Society, 495(2), 2332-2341. https://doi.org/10.1093/mnras/staa1315

Measurements of the cosmic far-infrared background (CIB) indicate that emission from many extragalactic phenomena, including star formation and black hole accretion, in the Universe can be obscured by dust. Resolving the CIB to study the population o... Read More about ALMACAL VII: First Interferometric Number Counts at 650 μm.

The e-MERGE Survey (e-MERLIN Galaxy Evolution Survey): overview and survey description (2020)
Journal Article
Venturi, T., Varenius, E., Swinbank, A., Simpson, J., Simpson, C., Serjeant, S., …Muxlow, T. (2020). The e-MERGE Survey (e-MERLIN Galaxy Evolution Survey): overview and survey description. Monthly Notices of the Royal Astronomical Society, 495(1), 1188-1208. https://doi.org/10.1093/mnras/staa1279

We present an overview and description of the e-MERGE Survey (e-MERLIN Galaxy Evolution Survey) Data Release 1 (DR1), a large program of high-resolution 1.5-GHz radio observations of the GOODS-N field comprising ∼140 h of observations with enhanced-M... Read More about The e-MERGE Survey (e-MERLIN Galaxy Evolution Survey): overview and survey description.

An ALMA survey of the SCUBA-2 CLS UDS field: Physical properties of 707 Sub-millimetre Galaxies (2020)
Journal Article
Dudzevičiūtė, U., Smail, I., Swinbank, A., Stach, S., Almaini, O., da Cunha, E., …van der Werf, P. (2020). An ALMA survey of the SCUBA-2 CLS UDS field: Physical properties of 707 Sub-millimetre Galaxies. Monthly Notices of the Royal Astronomical Society, 494(3), 3828-3860. https://doi.org/10.1093/mnras/staa769

We analyse the physical properties of a large, homogeneously selected sample of ALMA-located sub-millimetre galaxies (SMGs). This survey, AS2UDS, identified 707 SMGs across the ∼ 1 deg2 field, including ∼ 17 per cent which are undetected at K ≳ 25.7... Read More about An ALMA survey of the SCUBA-2 CLS UDS field: Physical properties of 707 Sub-millimetre Galaxies.

SuperCLASS – I. The super cluster assisted shear survey: Project overview and data release 1 (2020)
Journal Article
Whittaker, L., Tunbridge, B., Thomson, A., Thomas, D. B., Sanders, D. B., Peters, A., …Battye, R. A. (2020). SuperCLASS – I. The super cluster assisted shear survey: Project overview and data release 1. Monthly Notices of the Royal Astronomical Society, 495(2), 1706-1723. https://doi.org/10.1093/mnras/staa709

The SuperCLuster Assisted Shear Survey (SuperCLASS) is a legacy programme using the e-MERLIN interferometric array. The aim is to observe the sky at L-band (1.4 GHz) to a r.m.s. of 7μJybeam−1 over an area of ∼1deg2 centred on the Abell 981 superclust... Read More about SuperCLASS – I. The super cluster assisted shear survey: Project overview and data release 1.

The ALMA Spectroscopic Survey in the HUDF: The Cosmic Dust and Gas Mass Densities in Galaxies up to z ∼ 3 (2020)
Journal Article
Magnelli, B., Boogaard, L., Decarli, R., Gónzalez-López, J., Novak, M., Popping, G., …Weiss, A. (2020). The ALMA Spectroscopic Survey in the HUDF: The Cosmic Dust and Gas Mass Densities in Galaxies up to z ∼ 3. Astrophysical Journal, 892(1), Article 66. https://doi.org/10.3847/1538-4357/ab7897

Using the deepest 1.2 mm continuum map to date in the Hubble Ultra Deep Field, which was obtained as part of the ALMA Spectroscopic Survey (ASPECS) large program, we measure the cosmic density of dust and implied gas (H2+H I) mass in galaxies as a fu... Read More about The ALMA Spectroscopic Survey in the HUDF: The Cosmic Dust and Gas Mass Densities in Galaxies up to z ∼ 3.

Extended Hα over compact far-infrared continuum in dusty submillimeter galaxies (2020)
Journal Article
Chen, C., Harrison, C., Smail, I., Swinbank, A., Turner, O., Wardlow, J., …van der Werf, P. (2020). Extended Hα over compact far-infrared continuum in dusty submillimeter galaxies. Astronomy & Astrophysics, 635, Article A119. https://doi.org/10.1051/0004-6361/201936286

By using data from the Atacama Large Millimeter/submillimeter Array and near-infrared (NIR) integral field spectrographs, including both Spectrograph for INtegral Field Observations in the Near Infrared and K-band Multi Object Spectrograph on the Ver... Read More about Extended Hα over compact far-infrared continuum in dusty submillimeter galaxies.

SCUBA-2 Ultra Deep Imaging EAO Survey (Studies). III. Multiwavelength Properties, Luminosity Functions, and Preliminary Source Catalog of 450 μm Selected Galaxies (2020)
Journal Article
Lim, C., Wang, W., Smail, I., Scott, D., Chen, C., Chang, Y., …Wang, T. (2020). SCUBA-2 Ultra Deep Imaging EAO Survey (Studies). III. Multiwavelength Properties, Luminosity Functions, and Preliminary Source Catalog of 450 μm Selected Galaxies. Astrophysical Journal, 889(2), Article 80. https://doi.org/10.3847/1538-4357/ab607f

We construct a SCUBA-2 450 μm map in the COSMOS field that covers an area of 300 arcmin2 and reaches a 1σ noise level of 0.65 mJy in the deepest region. We extract 256 sources detected at 450 μm with signal-to-noise ratios >4.0 and analyze the physic... Read More about SCUBA-2 Ultra Deep Imaging EAO Survey (Studies). III. Multiwavelength Properties, Luminosity Functions, and Preliminary Source Catalog of 450 μm Selected Galaxies.

An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: Dust attenuation in high-redshift Lyman break Galaxies (2020)
Journal Article
Koprowski, M., Coppin, K., E. Geach, J., Dudzevičiūtė, U., Smail, I., Almaini, O., …Whitaker, K. (2020). An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: Dust attenuation in high-redshift Lyman break Galaxies. Monthly Notices of the Royal Astronomical Society, 492(4), 4927-4944. https://doi.org/10.1093/mnras/staa160

We analyse 870μm Atacama Large Millimetre Array (ALMA) dust continuum detections of 41 canonically-selected z ≃ 3 Lyman-break galaxies (LBGs), as well as 209 ALMA-undetected LBGs, in follow-up of SCUBA-2 mapping of the UKIDSS Ultra Deep Survey (UDS)... Read More about An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: Dust attenuation in high-redshift Lyman break Galaxies.

VIS3COS (2020)
Journal Article
Paulino-Afonso, A., Sobral, D., Darvish, B., Ribeiro, B., Smail, I., Best, P., …Cairns, J. (2020). VIS3COS. Astronomy & Astrophysics, 633, https://doi.org/10.1051/0004-6361/201834244

We present spectroscopic observations of 466 galaxies in and around a superstructure at z ∼ 0.84 targeted by the VIMOS Spectroscopic Survey of a Supercluster in the COSMOS field (VIS3COS). We use [OII]λ3727, Hδ, and Dn4000 to trace recent, medium-, a... Read More about VIS3COS.

From peculiar morphologies to Hubble-type spirals: the relation between galaxy dynamics and morphology in star-forming galaxies at z ∼ 1.5 (2019)
Journal Article
Gillman, S., Tiley, A., Swinbank, A., Harrison, C., Smail, I., Dudzevičiūtė, U., …Sweet, S. (2020). From peculiar morphologies to Hubble-type spirals: the relation between galaxy dynamics and morphology in star-forming galaxies at z ∼ 1.5. Monthly Notices of the Royal Astronomical Society, 492(1), 1492-1512. https://doi.org/10.1093/mnras/stz3576

We present an analysis of the gas dynamics of star–forming galaxies at z ∼ 1.5 using data from the KMOS Galaxy Evolution Survey (KGES). We quantify the morphology of the galaxies using HSTCANDELS imaging parametrically and non-parametrically. We comb... Read More about From peculiar morphologies to Hubble-type spirals: the relation between galaxy dynamics and morphology in star-forming galaxies at z ∼ 1.5.

Multi-wavelength Properties of Radio- and Machine-learning-identified Counterparts to Submillimeter Sources in S2COSMOS (2019)
Journal Article
Xia An, F., Simpson, J., Smail, I., Swinbank, A., Ma, C., Liu, D., …Smith, D. (2019). Multi-wavelength Properties of Radio- and Machine-learning-identified Counterparts to Submillimeter Sources in S2COSMOS. Astrophysical Journal, 886(1), Article 48. https://doi.org/10.3847/1538-4357/ab4d53

We identify multi-wavelength counterparts to 1147 submillimeter sources from the S2COSMOS SCUBA-2 survey of the COSMOS field by employing a recently developed radio+machine-learning method trained on a large sample of Atacama Large Millimeter/submill... Read More about Multi-wavelength Properties of Radio- and Machine-learning-identified Counterparts to Submillimeter Sources in S2COSMOS.

An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: High-resolution dust continuum morphologies and the link between sub-millimetre galaxies and spheroid formation (2019)
Journal Article
Gullberg, B., Smail, I., Swinbank, A., Dudzevičiūtė, U., Stach, S., Thomson, A., …Weiss, A. (2019). An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: High-resolution dust continuum morphologies and the link between sub-millimetre galaxies and spheroid formation. Monthly Notices of the Royal Astronomical Society, 490(4), 4956-4974. https://doi.org/10.1093/mnras/stz2835

We present an analysis of the morphology and profiles of the dust continuum emission in 153 bright sub-millimetre galaxies (SMGs) detected with ALMA at signal to noise ratios of >8 in high-resolution 0′′.18 (∼1 kpc) 870 μm maps. We measure sizes, sha... Read More about An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: High-resolution dust continuum morphologies and the link between sub-millimetre galaxies and spheroid formation.

The MUSE Ultra Deep Field (MUDF). II. Survey design and the gaseous properties of galaxy groups at 0.5 < z < 1.5 (2019)
Journal Article
Fossati, M., Fumagalli, M., Lofthouse, E., D’Odorico, V., Lusso, E., Cantalupo, S., …Theuns, T. (2019). The MUSE Ultra Deep Field (MUDF). II. Survey design and the gaseous properties of galaxy groups at 0.5 < z < 1.5. Monthly Notices of the Royal Astronomical Society, 490(1), 1451-1469. https://doi.org/10.1093/mnras/stz2693

We present the goals, design, and first results of the MUSE Ultra Deep Field (MUDF) survey, a large programme using the Multi Unit Spectroscopic Explorer (MUSE) instrument at the ESO Very Large Telescope. The MUDF survey is collecting ≈150 h on-sourc... Read More about The MUSE Ultra Deep Field (MUDF). II. Survey design and the gaseous properties of galaxy groups at 0.5 < z < 1.5.

Gas filaments of the cosmic web located around active galaxies in a protocluster (2019)
Journal Article
Umehata, H., Fumagalli, M., Smail, I., Matsuda, Y., Swinbank, A., Cantalupo, S., …Kohno, K. (2019). Gas filaments of the cosmic web located around active galaxies in a protocluster. Science, 366(6461), 97-100. https://doi.org/10.1126/science.aaw5949

Cosmological simulations predict the Universe contains a network of intergalactic gas filaments, within which galaxies form and evolve. However, the faintness of any emission from these filaments has limited tests of this prediction. We report the de... Read More about Gas filaments of the cosmic web located around active galaxies in a protocluster.

Radio Spectra and Sizes of Atacama Large Millimeter/submillimeter Array-identified Submillimeter Galaxies: Evidence of Age-related Spectral Curvature and Cosmic-Ray Diffusion? (2019)
Journal Article
Thomson, A., Smail, I., Swinbank, A., Simpson, J., Arumugam, V., Stach, S., …Wardlow, J. (2019). Radio Spectra and Sizes of Atacama Large Millimeter/submillimeter Array-identified Submillimeter Galaxies: Evidence of Age-related Spectral Curvature and Cosmic-Ray Diffusion?. Astrophysical Journal, 883(2), Article 204. https://doi.org/10.3847/1538-4357/ab32e7

We analyze the multifrequency radio spectral properties of 41 6 GHz-detected Atacama Large Millimeter/submillimeter Array (ALMA)-identified, submillimeter galaxies (SMGs), observed at 610 MHz, 1.4 GHz, and 6 GHz with the Giant Metrewave Radio Telesco... Read More about Radio Spectra and Sizes of Atacama Large Millimeter/submillimeter Array-identified Submillimeter Galaxies: Evidence of Age-related Spectral Curvature and Cosmic-Ray Diffusion?.

SILVERRUSH. VIII. Spectroscopic Identifications of Early Large-scale Structures with Protoclusters over 200 Mpc at z ∼ 6–7: Strong Associations of Dusty Star-forming Galaxies (2019)
Journal Article
Harikane, Y., Ouchi, M., Ono, Y., Fujimoto, S., Donevski, D., Shibuya, T., …Wang, W. (2019). SILVERRUSH. VIII. Spectroscopic Identifications of Early Large-scale Structures with Protoclusters over 200 Mpc at z ∼ 6–7: Strong Associations of Dusty Star-forming Galaxies. Astrophysical Journal, 883(2), Article 142. https://doi.org/10.3847/1538-4357/ab2cd5

We have obtained three-dimensional maps of the universe in ~200 × 200 × 80 comoving Mpc3 (cMpc3) volumes each at z = 5.7 and 6.6 based on a spectroscopic sample of 179 galaxies that achieves gsim80% completeness down to the Lyα luminosity of $\mathrm... Read More about SILVERRUSH. VIII. Spectroscopic Identifications of Early Large-scale Structures with Protoclusters over 200 Mpc at z ∼ 6–7: Strong Associations of Dusty Star-forming Galaxies.

ALMACAL VI: Molecular gas mass density across cosmic time via a blind search for intervening molecular absorbers (2019)
Journal Article
Klitsch, A., Péroux, C., Zwaan, M. A., Smail, I., Nelson, D., Popping, G., …Dutta, R. (2019). ALMACAL VI: Molecular gas mass density across cosmic time via a blind search for intervening molecular absorbers. Monthly Notices of the Royal Astronomical Society, 490(1), 1220-1230. https://doi.org/10.1093/mnras/stz2660

We are just starting to understand the physical processes driving the dramatic change in cosmic star-formation rate between z ∼ 2 and the present day. A quantity directly linked to star formation is the molecular gas density, which should be measured... Read More about ALMACAL VI: Molecular gas mass density across cosmic time via a blind search for intervening molecular absorbers.

The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Evolution of the Molecular Gas in CO-selected Galaxies (2019)
Journal Article
Aravena, M., Decarli, R., Gónzalez-López, J., Boogaard, L., Walter, F., Carilli, C., …Wisotzki, L. (2019). The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Evolution of the Molecular Gas in CO-selected Galaxies. Astrophysical Journal, 882(2), https://doi.org/10.3847/1538-4357/ab30df

We analyze the interstellar medium properties of a sample of 16 bright CO line emitting galaxies identified in the ALMA Spectroscopic Survey in the Hubble Ultra Deep Field (ASPECS) Large Program. This CO−selected galaxy sample is complemented by two... Read More about The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Evolution of the Molecular Gas in CO-selected Galaxies.

The Atacama Large Millimeter/submillimeter Array Spectroscopic Survey in the Hubble Ultra Deep Field: CO Emission Lines and 3 mm Continuum Sources (2019)
Journal Article
González-López, J., Decarli, R., Pavesi, R., Walter, F., Aravena, M., Carilli, C., …van der Werf, P. (2019). The Atacama Large Millimeter/submillimeter Array Spectroscopic Survey in the Hubble Ultra Deep Field: CO Emission Lines and 3 mm Continuum Sources. Astrophysical Journal, 882(2), https://doi.org/10.3847/1538-4357/ab3105

The Atacama Large Millimeter/submillimeter Array (ALMA) SPECtroscopic Survey in the Hubble Ultra Deep Field (HUDF) is an ALMA large program that obtained a frequency scan in the 3 mm band to detect emission lines from the molecular gas in distant gal... Read More about The Atacama Large Millimeter/submillimeter Array Spectroscopic Survey in the Hubble Ultra Deep Field: CO Emission Lines and 3 mm Continuum Sources.

The ALMA Spectroscopic Survey in the HUDF: Nature and Physical Properties of Gas-mass Selected Galaxies Using MUSE Spectroscopy (2019)
Journal Article
Boogaard, L. A., Decarli, R., González-López, J., van der Werf, P., Walter, F., Bouwens, R., …Wagg, J. (2019). The ALMA Spectroscopic Survey in the HUDF: Nature and Physical Properties of Gas-mass Selected Galaxies Using MUSE Spectroscopy. Astrophysical Journal, 882(2), https://doi.org/10.3847/1538-4357/ab3102

We discuss the nature and physical properties of gas-mass selected galaxies in the ALMA spectroscopic survey (ASPECS) of the Hubble Ultra Deep Field (HUDF). We capitalize on the deep optical integral-field spectroscopy from the Multi Unit Spectroscop... Read More about The ALMA Spectroscopic Survey in the HUDF: Nature and Physical Properties of Gas-mass Selected Galaxies Using MUSE Spectroscopy.

The ALMA Spectroscopic Survey in the HUDF: CO Luminosity Functions and the Molecular Gas Content of Galaxies through Cosmic History (2019)
Journal Article
Decarli, R., Walter, F., Gónzalez-López, J., Aravena, M., Boogaard, L., Carilli, C., …Wisotzki, L. (2019). The ALMA Spectroscopic Survey in the HUDF: CO Luminosity Functions and the Molecular Gas Content of Galaxies through Cosmic History. Astrophysical Journal, 882(2), https://doi.org/10.3847/1538-4357/ab30fe

We use the results from the ALMA large program ASPECS, the spectroscopic survey in the Hubble Ultra Deep Field (HUDF), to constrain CO luminosity functions of galaxies and the resulting redshift evolution of ρ(H2). The broad frequency range covered e... Read More about The ALMA Spectroscopic Survey in the HUDF: CO Luminosity Functions and the Molecular Gas Content of Galaxies through Cosmic History.

A machine-learning approach for identifying the counterparts of submillimetre galaxies and applications to the GOODS-North field (2019)
Journal Article
Liu, R. H., Hill, R., Scott, D., Almaini, O., An, F., Gubbels, C., …Stach, S. (2019). A machine-learning approach for identifying the counterparts of submillimetre galaxies and applications to the GOODS-North field. Monthly Notices of the Royal Astronomical Society, 489(2), 1770-1786. https://doi.org/10.1093/mnras/stz2228

Identifying the counterparts of submillimetre (submm) galaxies (SMGs) in multiwavelength images is a critical step towards building accurate models of the evolution of strongly star-forming galaxies in the early Universe. However, obtaining a statist... Read More about A machine-learning approach for identifying the counterparts of submillimetre galaxies and applications to the GOODS-North field.

The East Asian Observatory SCUBA-2 Survey of the COSMOS Field: Unveiling 1147 Bright Sub-millimeter Sources across 2.6 Square Degrees (2019)
Journal Article
Simpson, J., Smail, I., Swinbank, A., Chapman, S., Chen, C., Geach, J., …Wardlow, J. (2019). The East Asian Observatory SCUBA-2 Survey of the COSMOS Field: Unveiling 1147 Bright Sub-millimeter Sources across 2.6 Square Degrees. Astrophysical Journal, 880(1), Article 43. https://doi.org/10.3847/1538-4357/ab23ff

We present sensitive 850 μm imaging of the Cosmological Evolution Survey (COSMOS) field using 640 hr of new and archival observations taken with SCUBA-2 at the East Asian Observatory's James Clerk Maxwell Telescope. The SCUBA-2 COSMOS survey (S2COSMO... Read More about The East Asian Observatory SCUBA-2 Survey of the COSMOS Field: Unveiling 1147 Bright Sub-millimeter Sources across 2.6 Square Degrees.

Revealing the Stellar Mass and Dust Distributions of Submillimeter Galaxies at Redshift 2 (2019)
Journal Article
Lang, P., Schinnerer, E., Smail, I., Dudzevičiūtė, U., Swinbank, A., Liu, D., …Werf, P. V. D. (2019). Revealing the Stellar Mass and Dust Distributions of Submillimeter Galaxies at Redshift 2. Astrophysical Journal, 879(1), Article 54. https://doi.org/10.3847/1538-4357/ab1f77

We combine high-resolution ALMA and HST/CANDELS observations of 20 submillimeter galaxies (SMGs), predominantly from the AS2UDS survey at z sime 2, with bright rest-frame optical counterparts (${K}_{{\rm{s}}}\lesssim 22.9$) to investigate the resolve... Read More about Revealing the Stellar Mass and Dust Distributions of Submillimeter Galaxies at Redshift 2.

Two sub-millimetre bright protoclusters bounding the epoch of peak star-formation activity (2019)
Journal Article
Lacaille, K. M., Chapman, S. C., Smail, I., Steidel, C., Blain, A., Geach, J., …Sawicki, M. (2019). Two sub-millimetre bright protoclusters bounding the epoch of peak star-formation activity. Monthly Notices of the Royal Astronomical Society, 488(2), 1790-1812. https://doi.org/10.1093/mnras/stz1742

We present James Clerk Maxwell Telescope Submillimetre Common-User Bolometer Array 2 (SCUBA-2) 850 & 450 μm observations (σ850 ∼ 0.5 mJy, σ450 ∼ 5 mJy) of the HS1549+19 and HS1700+64 survey fields containing two of the largest known galaxy over-densi... Read More about Two sub-millimetre bright protoclusters bounding the epoch of peak star-formation activity.

The nature of sub-millimeter and highly star-forming galaxies in the eagle simulation (2019)
Journal Article
McAlpine, S., Smail, I., Bower, R. G., Swinbank, A., Trayford, J. W., Theuns, T., …Schaye, J. (2019). The nature of sub-millimeter and highly star-forming galaxies in the eagle simulation. Monthly Notices of the Royal Astronomical Society, 488(2), 2440-2454. https://doi.org/10.1093/mnras/stz1692

We exploit eagle, a cosmological hydrodynamical simulation, to reproduce the selection of the observed sub-millimeter (submm) galaxy population by selecting the model galaxies at z ≥ 1 with mock submm fluxes S850µm ≥ 1 mJy. We find a reasonable agree... Read More about The nature of sub-millimeter and highly star-forming galaxies in the eagle simulation.

The kiloparsec-scale gas kinematics in two star-forming galaxies at z ∼ 1.47 seen with ALMA and VLT-SINFONI (2019)
Journal Article
Molina, J., Ibar, E., Smail, I., Swinbank, A., Villard, E., Escala, A., …Hughes, T. (2019). The kiloparsec-scale gas kinematics in two star-forming galaxies at z ∼ 1.47 seen with ALMA and VLT-SINFONI. Monthly Notices of the Royal Astronomical Society, 487(4), 4856-4869. https://doi.org/10.1093/mnras/stz1643

We present Atacama Large Millimeter/submillimeter Array (ALMA) CO(J = 2 − 1) observations of two main-sequence star-forming galaxies at z ∼ 1.47 taken from the High-Z Emission Line Survey (HiZELS). These two systems have been previously reported to b... Read More about The kiloparsec-scale gas kinematics in two star-forming galaxies at z ∼ 1.47 seen with ALMA and VLT-SINFONI.

An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: Source catalogue and properties (2019)
Journal Article
Stach, S. M., Dudzevičiūtė, U., Smail, I., Swinbank, A., Geach, J., Simpson, J., …Werf, P. V. D. (2019). An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: Source catalogue and properties. Monthly Notices of the Royal Astronomical Society, 487(4), 4648-4668. https://doi.org/10.1093/mnras/stz1536

We present the catalogue and basic properties of sources in AS2UDS, an 870-μm continuum survey with the Atacama Large Millimetre/sub-millimetre Array (ALMA) of 716 single-dish sub-millimetre sources detected in the UKIDSS/UDS field by the SCUBA-2 Cos... Read More about An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: Source catalogue and properties.

ALMA Reveals Potential Evidence for Spiral Arms, Bars, and Rings in High-redshift Submillimeter Galaxies (2019)
Journal Article
Hodge, J., Smail, I., Walter, F., Cunha, E. D., Swinbank, A., Rybak, M., …Weiss, A. (2019). ALMA Reveals Potential Evidence for Spiral Arms, Bars, and Rings in High-redshift Submillimeter Galaxies. Astrophysical Journal, 876(2), Article 130. https://doi.org/10.3847/1538-4357/ab1846

We present subkiloparsec-scale mapping of the 870 μm ALMA continuum emission in six luminous (L IR ~ 5 × 1012 L ⊙) submillimeter galaxies (SMGs) from the ALESS survey of the Extended Chandra Deep Field South. Our high-fidelity 0farcs07-resolution ima... Read More about ALMA Reveals Potential Evidence for Spiral Arms, Bars, and Rings in High-redshift Submillimeter Galaxies.

The energetics of starburst-driven outflows at z ∼ 1 from KMOS (2019)
Journal Article
Swinbank, A., Harrison, C., Tiley, A., Johnson, H., Smail, I., Stott, J., …Sobral, D. (2019). The energetics of starburst-driven outflows at z ∼ 1 from KMOS. Monthly Notices of the Royal Astronomical Society, 487(1), 381-393. https://doi.org/10.1093/mnras/stz1275

We present an analysis of the gas outflow energetics from KMOS observations of 529 main-sequence star-forming galaxies at z 1 using broad, underlying Hα and forbid- den lines of [Nii] and [Sii]. Based on the stacked spectra for a sample with median s... Read More about The energetics of starburst-driven outflows at z ∼ 1 from KMOS.

Strong Far-ultraviolet Fields Drive the [C ii]/Far-infrared Deficit in z ∼ 3 Dusty, Star-forming Galaxies (2019)
Journal Article
Rybak, M., Rivera, G. C., Hodge, J., Smail, I., Walter, F., van der Werf, P., …Wardlow, J. (2019). Strong Far-ultraviolet Fields Drive the [C ii]/Far-infrared Deficit in z ∼ 3 Dusty, Star-forming Galaxies. Astrophysical Journal, 876(2), Article 112. https://doi.org/10.3847/1538-4357/ab0e0f

We present 0farcs15 (1 kpc) resolution ALMA observations of the [C ii] 157.74 μm line and rest-frame 160 μm continuum emission in two z ~ 3 dusty, star-forming galaxies—ALESS 49.1 and ALESS 57.1, combined with resolved CO (3–2) observations. In both... Read More about Strong Far-ultraviolet Fields Drive the [C ii]/Far-infrared Deficit in z ∼ 3 Dusty, Star-forming Galaxies.

The submillimetre view of massive clusters at z ∼ 0.8–1.6 (2019)
Journal Article
Cooke, E., Smail, I., Stach, S., Swinbank, A., Bower, R., Chen, C., …Thomson, A. (2019). The submillimetre view of massive clusters at z ∼ 0.8–1.6. Monthly Notices of the Royal Astronomical Society, 486(3), 3047-3058. https://doi.org/10.1093/mnras/stz955

We analyse 850 μm continuum observations of eight massive X-ray detected galaxy clusters at z ∼ 0.8–1.6 taken with SCUBA-2 on the James Clerk Maxwell Telescope. We find an average overdensity of 850 μm-selected sources of a factor of 4 ± 2 per cluste... Read More about The submillimetre view of massive clusters at z ∼ 0.8–1.6.

The SCUBA-2 Web Survey: I. Observations of CO(3–2) in hyper-luminous QSO fields (2019)
Journal Article
Hill, R., Chapman, S. C., Scott, D., Smail, I., Steidel, C. C., Krips, M., …Trainor, R. (2019). The SCUBA-2 Web Survey: I. Observations of CO(3–2) in hyper-luminous QSO fields. Monthly Notices of the Royal Astronomical Society, 485(1), 753-769. https://doi.org/10.1093/mnras/stz429

A primary goal of the SCUBA-2 Web survey is to perform tomography of the early inter-galactic medium by studying systems containing some of the brightest quasi-stellar objects (QSOs; 2.5  <  z  <  3.0) and nearby submillimetre galaxies. As a first st... Read More about The SCUBA-2 Web Survey: I. Observations of CO(3–2) in hyper-luminous QSO fields.

The Shapes of the Rotation Curves of Star-forming Galaxies Over the Last ≈ 10 Gyr (2019)
Journal Article
Tiley, A. L., Swinbank, A., Harrison, C., Smail, I., Turner, O., Schaller, M., …Magdis, G. (2019). The Shapes of the Rotation Curves of Star-forming Galaxies Over the Last ≈ 10 Gyr. Monthly Notices of the Royal Astronomical Society, 485(1), 934-960. https://doi.org/10.1093/mnras/stz428

We analyse maps of the spatially-resolved nebular emission of ≈1500 star-forming galaxies at z ≈ 0.6–2.2 from deep KMOS and MUSE observations to measure the average shape of their rotation curves. We use these to test claims for declining rotation cu... Read More about The Shapes of the Rotation Curves of Star-forming Galaxies Over the Last ≈ 10 Gyr.

COLDz: Shape of the CO Luminosity Function at High Redshift and the Cold Gas History of the Universe (2019)
Journal Article
Riechers, D. A., Pavesi, R., Sharon, C. E., Hodge, J. A., Decarli, R., Walter, F., …Wagg, J. (2019). COLDz: Shape of the CO Luminosity Function at High Redshift and the Cold Gas History of the Universe. Astrophysical Journal, 872(1), Article 7. https://doi.org/10.3847/1538-4357/aafc27

We report the first detailed measurement of the shape of the CO luminosity function at high redshift, based on >320 hr of the NSF's Karl G. Jansky Very Large Array (VLA) observations over an area of ~60 arcmin2 taken as part of the CO Luminosity Dens... Read More about COLDz: Shape of the CO Luminosity Function at High Redshift and the Cold Gas History of the Universe.

Overdensity of submillimeter galaxies around the z ≃ 2.3 MAMMOTH-1 nebula (2018)
Journal Article
Arrigoni Battaia, F., Chen, C., Fumagalli, M., Cai, Z., Calistro Rivera, G., Xu, J., …De Breuck, C. (2018). Overdensity of submillimeter galaxies around the z ≃ 2.3 MAMMOTH-1 nebula. Astronomy & Astrophysics, 620, Article A202. https://doi.org/10.1051/0004-6361/201834195

In the hierarchical model of structure formation, giant elliptical galaxies form through merging processes within the highest density peaks known as protoclusters. While high-redshift radio galaxies usually pinpoint the location of these environments... Read More about Overdensity of submillimeter galaxies around the z ≃ 2.3 MAMMOTH-1 nebula.

KROSS-SAMI: A Direct IFS Comparison of the Tully-Fisher Relation Across 8 Gyr Since z ≈ 1 (2018)
Journal Article
Tiley, A., Bureau, M., Cortese, L., Harrison, C., Johnson, H., Stott, J., …Richards, S. (2019). KROSS-SAMI: A Direct IFS Comparison of the Tully-Fisher Relation Across 8 Gyr Since z ≈ 1. Monthly Notices of the Royal Astronomical Society, 482(2), 2166-2188. https://doi.org/10.1093/mnras/sty2794

We construct Tully–Fisher relations (TFRs), from large samples of galaxies with spatially resolved H α emission maps from the K-band Multi-Object Spectrograph (KMOS) Redshift One Spectroscopic Survey (KROSS) at z ≈ 1. We compare these to data from th... Read More about KROSS-SAMI: A Direct IFS Comparison of the Tully-Fisher Relation Across 8 Gyr Since z ≈ 1.

ALMACAL V: absorption-selected galaxies with evidence for excited ISMs (2018)
Journal Article
Klitsch, A., Zwaan, M., Péroux, C., Smail, I., Oteo, I., Popping, G., …Biggs, A. (2018). ALMACAL V: absorption-selected galaxies with evidence for excited ISMs. Monthly Notices of the Royal Astronomical Society: Letters, 482(1), L65-L69. https://doi.org/10.1093/mnrasl/sly187

Gas-rich galaxies are selected efficiently via quasar absorption lines. Recently, a new perspective on such absorption-selected systems has opened up by studying the molecular gas content of absorber host galaxies using ALMA CO emission line observat... Read More about ALMACAL V: absorption-selected galaxies with evidence for excited ISMs.

SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES). II. Structural Properties and Near-infrared Morphologies of Faint Submillimeter Galaxies (2018)
Journal Article
Chang, Y., Ferraro, N., Wang, W., Lim, C., Toba, Y., An, F., …Urquhart, S. (2018). SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES). II. Structural Properties and Near-infrared Morphologies of Faint Submillimeter Galaxies. Astrophysical Journal, 865(2), Article 103. https://doi.org/10.3847/1538-4357/aadd18

We present structural parameters and morphological properties of faint 450 μm selected submillimeter galaxies (SMGs) from the JCMT Large Program, STUDIES, in the COSMOS-CANDELS region. Their properties are compared to an 850 μm selected and a matched... Read More about SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES). II. Structural Properties and Near-infrared Morphologies of Faint Submillimeter Galaxies.

The CO Luminosity Density at High-z (COLDz) Survey: A Sensitive, Large-area Blind Search for Low-J CO Emission from Cold Gas in the Early Universe with the Karl G. Jansky Very Large Array (2018)
Journal Article
Pavesi, R., Sharon, C. E., Riechers, D. A., Hodge, J. A., Decarli, R., Walter, F., …Wagg, J. (2018). The CO Luminosity Density at High-z (COLDz) Survey: A Sensitive, Large-area Blind Search for Low-J CO Emission from Cold Gas in the Early Universe with the Karl G. Jansky Very Large Array. Astrophysical Journal, 864(1), Article 49. https://doi.org/10.3847/1538-4357/aacb79

We describe the CO Luminosity Density at High-z (COLDz) survey, the first spectral line deep field targeting CO(1–0) emission from galaxies at z = 1.95–2.85 and CO(2–1) at z = 4.91–6.70. The main goal of COLDz is to constrain the cosmic density of mo... Read More about The CO Luminosity Density at High-z (COLDz) Survey: A Sensitive, Large-area Blind Search for Low-J CO Emission from Cold Gas in the Early Universe with the Karl G. Jansky Very Large Array.

Resolving the ISM at the Peak of Cosmic Star Formation with ALMA: The Distribution of CO and Dust Continuum in z ∼ 2.5 Submillimeter Galaxies (2018)
Journal Article
Rivera, G. C., Hodge, J., Smail, I., Swinbank, A., Weiss, A., Wardlow, J., …Werf, P. V. D. (2018). Resolving the ISM at the Peak of Cosmic Star Formation with ALMA: The Distribution of CO and Dust Continuum in z ∼ 2.5 Submillimeter Galaxies. Astrophysical Journal, 863(1), Article 56. https://doi.org/10.3847/1538-4357/aacffa

We use Atacama Large Millimeter Array (ALMA) observations of four submillimeter galaxies (SMGs) at z ~ 2–3 to investigate the spatially resolved properties of the interstellar medium (ISM) at scales of 1–5 kpc (0farcs1–0farcs6). The velocity fields o... Read More about Resolving the ISM at the Peak of Cosmic Star Formation with ALMA: The Distribution of CO and Dust Continuum in z ∼ 2.5 Submillimeter Galaxies.

Far-infrared Herschel SPIRE spectroscopy of lensed starbursts reveals physical conditions of ionized gas (2018)
Journal Article
Zhang, Z., Ivison, R., George, R., Zhao, Y., Dunne, L., Herrera-Camus, R., …van der Werf, P. (2018). Far-infrared Herschel SPIRE spectroscopy of lensed starbursts reveals physical conditions of ionized gas. Monthly Notices of the Royal Astronomical Society, 481(1), 59-97. https://doi.org/10.1093/mnras/sty2082

The most intensively star-forming galaxies are extremely luminous at far-infrared (FIR) wavelengths, highly obscured at optical and ultraviolet wavelengths, and lie at z ≥ 1–3. We present a programme of FIR spectroscopic observations with the SPIRE F... Read More about Far-infrared Herschel SPIRE spectroscopy of lensed starbursts reveals physical conditions of ionized gas.

A Machine-learning Method for Identifying Multiwavelength Counterparts of Submillimeter Galaxies: Training and Testing Using AS2UDS and ALESS (2018)
Journal Article
An, F. X., Stach, S., Smail, I., Swinbank, A., Almaini, O., Simpson, C., …Coppin, K. (2018). A Machine-learning Method for Identifying Multiwavelength Counterparts of Submillimeter Galaxies: Training and Testing Using AS2UDS and ALESS. Astrophysical Journal, 862(2), Article 101. https://doi.org/10.3847/1538-4357/aacdaa

We describe the application of supervised machine-learning algorithms to identify the likely multiwavelength counterparts to submillimeter sources detected in panoramic, single-dish submillimeter surveys. As a training set, we employ a sample of 695... Read More about A Machine-learning Method for Identifying Multiwavelength Counterparts of Submillimeter Galaxies: Training and Testing Using AS2UDS and ALESS.

An ALMA Survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS Field: Identifying Candidate z ∼ 4.5 [C II] Emitters (2018)
Journal Article
Cooke, E., Smail, I., Swinbank, A., Stach, S., An, F. X., Gullberg, B., …Werf, P. V. D. (2018). An ALMA Survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS Field: Identifying Candidate z ∼ 4.5 [C II] Emitters. Astrophysical Journal, 861(2), Article 100. https://doi.org/10.3847/1538-4357/aac6ba

We report the results of a search for serendipitous [C ii] 157.74 μm emitters at z sime 4.4–4.7 using the Atacama Large Millimeter/submillimeter Array (ALMA). The search exploits the AS2UDS continuum survey, which covers ~50 arcmin2 of the sky toward... Read More about An ALMA Survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS Field: Identifying Candidate z ∼ 4.5 [C II] Emitters.

An ALMA Survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS Field: Number Counts of Submillimeter Galaxies (2018)
Journal Article
Stach, S. M., Smail, I., Swinbank, A., Simpson, J., Geach, J., An, F. X., …Werf, P. V. D. (2018). An ALMA Survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS Field: Number Counts of Submillimeter Galaxies. Astrophysical Journal, 860(2), Article 161. https://doi.org/10.3847/1538-4357/aac5e5

We report the first results of AS2UDS, an 870 μm continuum survey with the Atacama Large Millimeter/Submillimeter Array (ALMA) of a total area of ~50 arcmin2 comprising a complete sample of 716 submillimeter sources drawn from the SCUBA-2 Cosmology L... Read More about An ALMA Survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS Field: Number Counts of Submillimeter Galaxies.

The Discovery of a New Massive Molecular Gas Component Associated with the Submillimeter Galaxy SMM J02399-0136 (2018)
Journal Article
Frayer, D., Maddalena, R., Ivison, R., Smail, I., Blain, A., & Vanden Bout, P. (2018). The Discovery of a New Massive Molecular Gas Component Associated with the Submillimeter Galaxy SMM J02399-0136. Astrophysical Journal, 860(2), Article 87. https://doi.org/10.3847/1538-4357/aac49a

We present CO(1–0), CO(3–2), and CO(7–6) observations using the Green Bank Telescope (GBT) and the Atacama Large Millimeter Array (ALMA) of the z = 2.8 submillimeter galaxy SMM J02399−0136. This was the first submillimeter-selected galaxy discovered... Read More about The Discovery of a New Massive Molecular Gas Component Associated with the Submillimeter Galaxy SMM J02399-0136.

An ALMA survey of CO in submillimetre galaxies: companions, triggering, and the environment in blended sources (2018)
Journal Article
Wardlow, J., Simpson, J., Smail, I., Swinbank, A., Blain, A., Brandt, W., …van der Werf, P. (2018). An ALMA survey of CO in submillimetre galaxies: companions, triggering, and the environment in blended sources. Monthly Notices of the Royal Astronomical Society, 479(3), 3879-3891. https://doi.org/10.1093/mnras/sty1526

We present ALMA observations of the mid-J 12CO emission from six single-dish selected 870-μm sources in the Extended Chandra Deep Field-South and UKIDSS Ultra-Deep Survey fields. These six single-dish submillimetre sources were selected based on prev... Read More about An ALMA survey of CO in submillimetre galaxies: companions, triggering, and the environment in blended sources.

The Dust and [C ii] Morphologies of Redshift ∼4.5 Sub-millimeter Galaxies at ∼200 pc Resolution: The Absence of Large Clumps in the Interstellar Medium at High-redshift (2018)
Journal Article
Gullberg, B., Swinbank, A., Smail, I., Biggs, A., Bertoldi, F., Breuck, C. D., …Weiss, A. (2018). The Dust and [C ii] Morphologies of Redshift ∼4.5 Sub-millimeter Galaxies at ∼200 pc Resolution: The Absence of Large Clumps in the Interstellar Medium at High-redshift. Astrophysical Journal, 859(1), Article 12. https://doi.org/10.3847/1538-4357/aabe8c

We present deep, high-resolution (0 03, 200 pc) ALMA Band 7 observations covering the dust continuum and [C II] λ157.7 μm emission in four z ∼ 4.4–4.8 sub-millimeter galaxies (SMGs) selected from the ALESS and AS2UDS surveys. The data show that the r... Read More about The Dust and [C ii] Morphologies of Redshift ∼4.5 Sub-millimeter Galaxies at ∼200 pc Resolution: The Absence of Large Clumps in the Interstellar Medium at High-redshift.

The XMM-SERVS survey: new XMM-Newton point-source catalogue for the XMM-LSS field (2018)
Journal Article
Chen, C., Brandt, W., Luo, B., Ranalli, P., Yang, G., Alexander, D., …Trump, J. (2018). The XMM-SERVS survey: new XMM-Newton point-source catalogue for the XMM-LSS field. Monthly Notices of the Royal Astronomical Society, 478, 2132-2163. https://doi.org/10.1093/mnras/sty1036

We present an X-ray point-source catalogue from the XMM-Large Scale Structure (XMM-LSS) survey region, one of the XMM-Spitzer Extragalactic Representative Volume Survey (XMM-SERVS) fields. We target the XMM-LSS region with 1.3 Ms of new XMM–Newton AO... Read More about The XMM-SERVS survey: new XMM-Newton point-source catalogue for the XMM-LSS field.

The clustering of H $\beta$ + [O III] and [O II] emitters since z \tilde 5: dependencies with line luminosity and stellar mass (2018)
Journal Article
Khostovan, A., Sobral, D., Mobasher, B., Best, P., Smail, I., Matthee, J., …Stott, J. (2018). The clustering of H $\beta$ + [O III] and [O II] emitters since z \tilde 5: dependencies with line luminosity and stellar mass. Monthly Notices of the Royal Astronomical Society, 478(3), 2999-3015. https://doi.org/10.1093/mnras/sty925

We investigate the clustering properties of ∼7000 H β + [O III] and [O II] narrowband-selected emitters at z ∼ 0.8–4.7 from the High-z Emission Line Survey. We find clustering lengths, r0, of 1.5–4.0 h−1 Mpc and minimum dark matter halo masses of 101... Read More about The clustering of H $\beta$ + [O III] and [O II] emitters since z \tilde 5: dependencies with line luminosity and stellar mass.

The nature of luminous Ly α emitters at z ∼ 2–3: maximal dust-poor starbursts and highly ionizing AGN (2018)
Journal Article
Sobral, D., Matthee, J., Darvish, B., Smail, I., Best, P. N., Alegre, L., …Oteo, I. (2018). The nature of luminous Ly α emitters at z ∼ 2–3: maximal dust-poor starbursts and highly ionizing AGN. Monthly Notices of the Royal Astronomical Society, 477(2), 2817-2840. https://doi.org/10.1093/mnras/sty782

Deep narrow-band surveys have revealed a large population of faint Ly α emitters (LAEs) in the distant Universe, but relatively little is known about the most luminous sources ( LLyα≳1042.7  erg s−1; LLyα≳L∗Lyα ). Here we present the spectroscopic fo... Read More about The nature of luminous Ly α emitters at z ∼ 2–3: maximal dust-poor starbursts and highly ionizing AGN.

High-resolution SMA imaging of bright submillimetre sources from the SCUBA-2 Cosmology Legacy Survey (2018)
Journal Article
Hill, R., Chapman, S. C., Scott, D., Petitpas, G., Smail, I., Chapin, E. L., …Wilner, D. J. (2018). High-resolution SMA imaging of bright submillimetre sources from the SCUBA-2 Cosmology Legacy Survey. Monthly Notices of the Royal Astronomical Society, 477(2), 2042-2067. https://doi.org/10.1093/mnras/sty746

We have used the Submillimeter Array (SMA) at 860 µm to observe the brightest sources in the Submillimeter Common User Bolometer Array-2 (SCUBA-2) Cosmology Legacy Survey (S2CLS). The goal of this survey is to exploit the large field of the S2CLS alo... Read More about High-resolution SMA imaging of bright submillimetre sources from the SCUBA-2 Cosmology Legacy Survey.

The dependence of galaxy clustering on stellar mass, star-formation rate and redshift at z = 0.8–2.2, with HiZELS (2018)
Journal Article
Cochrane, R., Best, P., Sobral, D., Smail, I., Geach, J., Stott, J., & Wake, D. (2018). The dependence of galaxy clustering on stellar mass, star-formation rate and redshift at z = 0.8–2.2, with HiZELS. Monthly Notices of the Royal Astronomical Society, 475(3), 3730-3745. https://doi.org/10.1093/mnras/stx3345

The deep, near-infrared narrow-band survey HiZELS has yielded robust samples of H α-emitting star-forming galaxies within narrow redshift slices at z = 0.8,  1.47 and 2.23. In this paper, we distinguish the stellar mass and star-formation rate (SFR)... Read More about The dependence of galaxy clustering on stellar mass, star-formation rate and redshift at z = 0.8–2.2, with HiZELS.

Molecular gas in the Herschel-selected strongly lensed submillimeter galaxies at z ~ 2–4 as probed by multi-J CO lines (2017)
Journal Article
Yang, C., Omont, A., Beelen, A., Gao, Y., van der Werf, P., Gavazzi, R., …Smail, I. (2017). Molecular gas in the Herschel-selected strongly lensed submillimeter galaxies at z ~ 2–4 as probed by multi-J CO lines. Astronomy & Astrophysics, 608, https://doi.org/10.1051/0004-6361/201731391

We present the IRAM-30 m observations of multiple-J CO (Jup mostly from 3 up to 8) and [C I](3P2 → 3P1) ([C I](2–1) hereafter) line emission in a sample of redshift ~2–4 submillimeter galaxies (SMGs). These SMGs are selected among the brightest-lense... Read More about Molecular gas in the Herschel-selected strongly lensed submillimeter galaxies at z ~ 2–4 as probed by multi-J CO lines.

ALMACAL – III. A combined ALMA and MUSE survey for neutral, molecular, and ionized gas in an H i-absorption-selected system (2017)
Journal Article
Klitsch, A., Péroux, C., Zwaan, M., Smail, I., Oteo, I., Biggs, A., …Swinbank, A. (2018). ALMACAL – III. A combined ALMA and MUSE survey for neutral, molecular, and ionized gas in an H i-absorption-selected system. Monthly Notices of the Royal Astronomical Society, 475(1), 492-507. https://doi.org/10.1093/mnras/stx3184

Studying the flow of baryons into and out of galaxies is an important part of understanding the evolution of galaxies over time. We present a detailed case study of the environment around an intervening Ly α absorption line system at zabs = 0.633, se... Read More about ALMACAL – III. A combined ALMA and MUSE survey for neutral, molecular, and ionized gas in an H i-absorption-selected system.

The KMOS Redshift One Spectroscopic Survey (KROSS): the origin of disc turbulence in z ≈ 1 star-forming galaxies (2017)
Journal Article
Johnson, H., Harrison, C., Swinbank, A., Tiley, A., Stott, J., Bower, R., …Richards, S. (2018). The KMOS Redshift One Spectroscopic Survey (KROSS): the origin of disc turbulence in z ≈ 1 star-forming galaxies. Monthly Notices of the Royal Astronomical Society, 474(4), 5076-5104. https://doi.org/10.1093/mnras/stx3016

We analyse the velocity dispersion properties of 472 z ∼ 0.9 star-forming galaxies observed as part of the KMOS Redshift One Spectroscopic Survey (KROSS). The majority of this sample is rotationally dominated (83 ± 5 per cent with vC/σ0 > 1) but also... Read More about The KMOS Redshift One Spectroscopic Survey (KROSS): the origin of disc turbulence in z ≈ 1 star-forming galaxies.

SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES): Faint-end Counts at 450 μm (2017)
Journal Article
Wang, W., Lin, W., Lim, C., Smail, I., Chapman, S. C., Zheng, X. Z., …Wardlow, J. L. (2017). SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES): Faint-end Counts at 450 μm. Astrophysical Journal, 850(1), Article 37. https://doi.org/10.3847/1538-4357/aa911b

The SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES) is a three-year JCMT Large Program aiming to reach the 450 μm confusion limit in the COSMOS-CANDELS region to study a representative sample of the high-redshift far-infrared galaxy population that g... Read More about SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES): Faint-end Counts at 450 μm.

ALMA Pinpoints a Strong Overdensity of U/LIRGs in the Massive Cluster XCS J2215 at z = 1.46 (2017)
Journal Article
Stach, S. M., Swinbank, A., Smail, I., Hilton, M., Simpson, J., & Cooke, E. (2017). ALMA Pinpoints a Strong Overdensity of U/LIRGs in the Massive Cluster XCS J2215 at z = 1.46. Astrophysical Journal, 849(2), Article 154. https://doi.org/10.3847/1538-4357/aa93f6

We surveyed the core regions of the z = 1.46 cluster XCS J2215.9−1738 with the Atacama Large Millimeter Array (ALMA) and the MUSE-GALACSI spectrograph on the Very Large Telescope (VLT). We obtained high spatial resolution observations with ALMA of th... Read More about ALMA Pinpoints a Strong Overdensity of U/LIRGs in the Massive Cluster XCS J2215 at z = 1.46.

The Interstellar Medium in [O iii]-selected Star-forming Galaxies at z ∼ 3.2 (2017)
Journal Article
Suzuki, T. L., Kodama, T., Onodera, M., Shimakawa, R., Hayashi, M., Tadaki, K., …Yamamoto, M. (2017). The Interstellar Medium in [O iii]-selected Star-forming Galaxies at z ∼ 3.2. Astrophysical Journal, 849(1), Article 39. https://doi.org/10.3847/1538-4357/aa8df3

We present new results from near-infrared spectroscopy with Keck/MOSFIRE of [O III]-selected galaxies at z ~ 3.2. With our H and K band spectra, we investigate the interstellar medium (ISM) conditions, such as ionization states and gas metallicities.... Read More about The Interstellar Medium in [O iii]-selected Star-forming Galaxies at z ∼ 3.2.

A Spatially Resolved Study of Cold Dust, Molecular Gas, H ii Regions, and Stars in the z = 2.12 Submillimeter Galaxy ALESS67.1 (2017)
Journal Article
Chen, C., Hodge, J., Smail, I., Swinbank, A., Walter, F., Simpson, J., …Werf, P. V. D. (2017). A Spatially Resolved Study of Cold Dust, Molecular Gas, H ii Regions, and Stars in the z = 2.12 Submillimeter Galaxy ALESS67.1. Astrophysical Journal, 846(2), Article 108. https://doi.org/10.3847/1538-4357/aa863a

We present detailed studies of a z = 2.12 submillimeter galaxy, ALESS67.1, using sub-arcsecond resolution ALMA, adaptive optics-aided VLT/SINFONI, and Hubble Space Telescope (HST)/CANDELS data to investigate the kinematics and spatial distributions o... Read More about A Spatially Resolved Study of Cold Dust, Molecular Gas, H ii Regions, and Stars in the z = 2.12 Submillimeter Galaxy ALESS67.1.

An Imperfectly Passive Nature: Bright Submillimeter Emission from Dust-obscured Star Formation in the z = 3.717 “Passive” System, ZF 20115 (2017)
Journal Article
Simpson, J., Smail, I., Wang, W., Riechers, D., Dunlop, J., Ao, Y., …Zheng, X. (2017). An Imperfectly Passive Nature: Bright Submillimeter Emission from Dust-obscured Star Formation in the z = 3.717 “Passive” System, ZF 20115. Astrophysical Journal Letters, 844(1), Article L10. https://doi.org/10.3847/2041-8213/aa7cf2

The identification of high-redshift, massive galaxies with old stellar populations may pose challenges to some models of galaxy formation. However, to securely classify a galaxy as quiescent, it is necessary to exclude significant ongoing star format... Read More about An Imperfectly Passive Nature: Bright Submillimeter Emission from Dust-obscured Star Formation in the z = 3.717 “Passive” System, ZF 20115.

The eMERGE Survey - I: Very Large Array 5.5 GHz observations of the GOODS-North Field (2017)
Journal Article
Guidetti, D., Bondi, M., Prandoni, I., Muxlow, T., Beswick, R., Wrigley, N., …Argo, M. (2017). The eMERGE Survey - I: Very Large Array 5.5 GHz observations of the GOODS-North Field. Monthly Notices of the Royal Astronomical Society, 471(1), 210-226. https://doi.org/10.1093/mnras/stx1162

We present new observations of the GOODS-N field obtained at 5.5 GHz with the Karl G. Jansky Very Large Array. The central region of the field was imaged to a median rms of 3 μJy beam−1 with a resolution of 0.5 arcsec. From a 14-arcmin diameter regio... Read More about The eMERGE Survey - I: Very Large Array 5.5 GHz observations of the GOODS-North Field.

Boötes-HiZELS: an optical to near-infrared survey of emission-line galaxies at z = 0.4-4.7 (2017)
Journal Article
Matthee, J., Sobral, D., Best, P., Smail, I., Bian, F., Darvish, B., …Fan, X. (2017). Boötes-HiZELS: an optical to near-infrared survey of emission-line galaxies at z = 0.4-4.7. Monthly Notices of the Royal Astronomical Society, 471(1), 629-649. https://doi.org/10.1093/mnras/stx1569

We present a sample of ∼1000 emission-line galaxies at z = 0.4–4.7 from the ∼0.7deg2 High-z Emission-Line Survey in the Boötes field identified with a suite of six narrow-band filters at ≈0.4–2.1 μm. These galaxies have been selected on their Ly α (7... Read More about Boötes-HiZELS: an optical to near-infrared survey of emission-line galaxies at z = 0.4-4.7.

An ALMA Survey of Submillimeter Galaxies in the Extended Chandra Deep Field South: Spectroscopic Redshifts (2017)
Journal Article
Danielson, A., Swinbank, A., Smail, I., Simpson, J., Casey, C., Chapman, S., …van der Werf, P. (2017). An ALMA Survey of Submillimeter Galaxies in the Extended Chandra Deep Field South: Spectroscopic Redshifts. Astrophysical Journal, 840(2), Article 78. https://doi.org/10.3847/1538-4357/aa6caf

We present spectroscopic redshifts of {\text{}}{S}870μ {{m}} ≳ 2 mJy submillimeter galaxies (SMGs), which have been identified from the ALMA follow-up observations of 870 μm detected sources in the Extended Chandra Deep Field South (the ALMA-LESS sur... Read More about An ALMA Survey of Submillimeter Galaxies in the Extended Chandra Deep Field South: Spectroscopic Redshifts.

ALMA deep field in SSA22: Blindly detected CO emitters and [C ii] emitter candidates (2017)
Journal Article
Hayatsu, N., Matsuda, Y., Umehata, H., Yoshida, N., Smail, I., Swinbank, A., …Yamada, T. (2017). ALMA deep field in SSA22: Blindly detected CO emitters and [C ii] emitter candidates. Publications of Astronomical Society of Japan, 69(3), https://doi.org/10.1093/pasj/psx018

We report the identification of four millimeter line-emitting galaxies with the Atacama Large Milli/submillimeter Array (ALMA) in SSA22 Field (ADF22). We analyze the ALMA 1.1-mm survey data, with an effective survey area of 5 arcmin2, frequency range... Read More about ALMA deep field in SSA22: Blindly detected CO emitters and [C ii] emitter candidates.

The Hawaii SCUBA-2 Lensing Cluster Survey: Radio-detected Submillimeter Galaxies in the HST Frontier Fields (2017)
Journal Article
Hsu, L., Desai, V., Murphy, E., Cowie, L., Heywood, I., Momjian, E., …Smail, I. (2017). The Hawaii SCUBA-2 Lensing Cluster Survey: Radio-detected Submillimeter Galaxies in the HST Frontier Fields. Astrophysical Journal, 840(1), Article 29. https://doi.org/10.3847/1538-4357/aa6ba0

In this second paper of the Hawaii SCUBA-2 Lensing Cluster Survey series, we cross-match SCUBA-2 maps with 3 and 6 GHz images from the Janksy-VLA Frontier Fields Legacy Survey for three cluster fields, MACS J0416.1--2403, MACS J0717.5+3745, and MACS... Read More about The Hawaii SCUBA-2 Lensing Cluster Survey: Radio-detected Submillimeter Galaxies in the HST Frontier Fields.

The H α luminosity-dependent clustering of star-forming galaxies from z ∼ 0.8 to ∼2.2 with HiZELS (2017)
Journal Article
Cochrane, R., Best, P., Sobral, D., Smail, I., Wake, D., Stott, J., & Geach, J. (2017). The H α luminosity-dependent clustering of star-forming galaxies from z ∼ 0.8 to ∼2.2 with HiZELS. Monthly Notices of the Royal Astronomical Society, 469(3), 2913-2932. https://doi.org/10.1093/mnras/stx957

We present clustering analyses of identically selected star-forming galaxies in three narrow redshift slices (at z = 0.8, 1.47 and 2.23), from the High-Redshift(Z) Emission Line Survey (HiZELS), a deep, near-infrared narrow-band survey. The HiZELS sa... Read More about The H α luminosity-dependent clustering of star-forming galaxies from z ∼ 0.8 to ∼2.2 with HiZELS.

The SCUBA-2 Cosmology Legacy Survey: Multi-wavelength Properties of ALMA-identified Submillimeter Galaxies in UKIDSS UDS (2017)
Journal Article
Simpson, J., Smail, I., Swinbank, A., Ivison, R., Dunlop, J., Geach, J., …van der Werf, P. (2017). The SCUBA-2 Cosmology Legacy Survey: Multi-wavelength Properties of ALMA-identified Submillimeter Galaxies in UKIDSS UDS. Astrophysical Journal, 839(1), Article 58. https://doi.org/10.3847/1538-4357/aa65d0

We present a multi-wavelength analysis of 52 submillimeter galaxies (SMGs), identified using ALMA 870 μm continuum imaging in a pilot program to precisely locate bright SCUBA-2-selected submillimeter sources in the UKIDSS Ultra Deep Survey (UDS) fiel... Read More about The SCUBA-2 Cosmology Legacy Survey: Multi-wavelength Properties of ALMA-identified Submillimeter Galaxies in UKIDSS UDS.

Evolution of Dust-obscured Star Formation and Gas to z = 2.2 from HiZELS (2017)
Journal Article
Thomson, A., Simpson, J., Smail, I., Swinbank, A., Best, P., Sobral, D., …Johnson, H. (2017). Evolution of Dust-obscured Star Formation and Gas to z = 2.2 from HiZELS. Astrophysical Journal, 838(2), Article 119. https://doi.org/10.3847/1538-4357/aa61a6

We investigate the far-infrared properties of galaxies selected via deep, narrow-band imaging of the Hα emission line in four redshift slices from z=0.40--2.23 over ∼1deg2 as part of the High-redshift Emission Line Survey (HiZELS). We use a stacking... Read More about Evolution of Dust-obscured Star Formation and Gas to z = 2.2 from HiZELS.

ALMACAL II: Extreme Star Formation Rate Densities in Dusty Starbursts Revealed by ALMA 20 mas Resolution Imaging (2017)
Journal Article
Oteo, I., Zwaan, M., Ivison, R., Smail, I., & Biggs, A. (2017). ALMACAL II: Extreme Star Formation Rate Densities in Dusty Starbursts Revealed by ALMA 20 mas Resolution Imaging. Astrophysical Journal, 837(2), Article 182. https://doi.org/10.3847/1538-4357/aa5da4

We present ultrahigh spatial resolution (˜20 mas or 150 pc) ALMA observations of the dust continuum at 920 μm and 1.2 mm in two submillimeter sources at z = 3.442, ALMACAL-1 (A-1: {S}870μ {{m}}=6.5+/- 0.2 {mJy}) and ALMACAL-2 (A-2: {S}870μ {{m}}=4.4+... Read More about ALMACAL II: Extreme Star Formation Rate Densities in Dusty Starbursts Revealed by ALMA 20 mas Resolution Imaging.

A gravitationally boosted MUSE survey for emission-line galaxies at z ≳ 5 behind the massive cluster RCS 0224 (2017)
Journal Article
Smit, R., Swinbank, A., Massey, R., Richard, J., Smail, I., & Kneib, J. (2017). A gravitationally boosted MUSE survey for emission-line galaxies at z ≳ 5 behind the massive cluster RCS 0224. Monthly Notices of the Royal Astronomical Society, 476(3), 3306-3323. https://doi.org/10.1093/mnras/stx245

We present a Very Large Telescope/Multi Unit Spectroscopic Explorer (MUSE) survey of lensed high-redshift galaxies behind the z = 0.77 cluster RCS 0224−0002. We study the detailed internal properties of a highly magnified (μ ∼ 29) z = 4.88 galaxy see... Read More about A gravitationally boosted MUSE survey for emission-line galaxies at z ≳ 5 behind the massive cluster RCS 0224.

The KMOS Redshift One Spectroscopic Survey (KROSS): rotational velocities and angular momentum of z ≈ 0.9 galaxies (2017)
Journal Article
Harrison, C., Johnson, H., Swinbank, A., Stott, J., Bower, R., Smail, I., …Magdis, G. (2017). The KMOS Redshift One Spectroscopic Survey (KROSS): rotational velocities and angular momentum of z ≈ 0.9 galaxies. Monthly Notices of the Royal Astronomical Society, 467(2), 1965-1983. https://doi.org/10.1093/mnras/stx217

We present dynamical measurements for 586 Hα detected star-forming galaxies from the KMOS (K-band Multi-Object Spectrograph) Redshift One Spectroscopic Survey (KROSS). The sample represents typical star-forming galaxies at this redshift (z = 0.6–1.0)... Read More about The KMOS Redshift One Spectroscopic Survey (KROSS): rotational velocities and angular momentum of z ≈ 0.9 galaxies.

Angular momentum evolution of galaxies over the past 10 Gyr: a MUSE and KMOS dynamical survey of 400 star-forming galaxies from z = 0.3 to 1.7 (2017)
Journal Article
Swinbank, M., Harrison, C., Trayford, J., Schaller, M., Smail, I., Schaye, J., …Stott, J. (2017). Angular momentum evolution of galaxies over the past 10 Gyr: a MUSE and KMOS dynamical survey of 400 star-forming galaxies from z = 0.3 to 1.7. Monthly Notices of the Royal Astronomical Society, 467(3), 3140-3159. https://doi.org/10.1093/mnras/stx201

We present a MUSE and KMOS dynamical study 405 star-forming galaxies at redshift z = 0.28–1.65 (median redshift z¯= 0.84). Our sample is representative of the star-forming “main-sequence”, with star-formation rates of SFR = 0.1–30M⊙ yr−1 and stellar... Read More about Angular momentum evolution of galaxies over the past 10 Gyr: a MUSE and KMOS dynamical survey of 400 star-forming galaxies from z = 0.3 to 1.7.

The AT-LESS CO(1–0) survey of submillimetre galaxies in the Extended Chandra Deep Field South: first results on cold molecular gas in galaxies at z ∼ 2 (2017)
Journal Article
Huynh, M. T., Emonts, B., Kimball, A., Seymour, N., Smail, I., Swinbank, A., …Wardlow, J. (2017). The AT-LESS CO(1–0) survey of submillimetre galaxies in the Extended Chandra Deep Field South: first results on cold molecular gas in galaxies at z ∼ 2. Monthly Notices of the Royal Astronomical Society, 467(1), 1222-1230. https://doi.org/10.1093/mnras/stx156

We present the first results from our ongoing Australia Telescope Compact Array survey of 12CO(1–0) in Atacama Large Millimeter Array (ALMA)-identified submillimetre galaxies (SMGs) in the Extended Chandra Deep Field South. Strong detections of 12CO(... Read More about The AT-LESS CO(1–0) survey of submillimetre galaxies in the Extended Chandra Deep Field South: first results on cold molecular gas in galaxies at z ∼ 2.

ALMA Deep Field in SSA22: Source Catalog and Number Counts (2017)
Journal Article
Umehata, H., Tamura, Y., Kohno, K., Ivison, R., Smail, I., Hatsukade, B., …Kubo, M. (2017). ALMA Deep Field in SSA22: Source Catalog and Number Counts. Astrophysical Journal, 835(1), Article 98. https://doi.org/10.3847/1538-4357/835/1/98

We present results from a deep 2' × 3' (comoving scale of 3.7 Mpc × 5.5 Mpc at z = 3) survey at 1.1 mm, taken with the Atacama Large Millimeter/submillimeter Array (ALMA) in the SSA22 field. We observe the core region of a z = 3.09 protocluster, achi... Read More about ALMA Deep Field in SSA22: Source Catalog and Number Counts.

ALMA Reveals Strong [C II] Emission in a Galaxy Embedded in a Giant Lyα Blob at z = 3.1 (2017)
Journal Article
Umehata, H., Matsuda, Y., Tamura, Y., Kohno, K., Smail, I., Ivison, R., …Ouchi, M. (2017). ALMA Reveals Strong [C II] Emission in a Galaxy Embedded in a Giant Lyα Blob at z = 3.1. Astrophysical Journal Letters, 834(2), Article L16. https://doi.org/10.3847/2041-8213/834/2/l16

We report the result from observations conducted with the Atacama Large Millimeter/submillimeter Array (ALMA) to detect [C ii] 158 μm fine structure line emission from galaxies embedded in one of the most spectacular Lyα blobs (LABs) at z = 3.1, SSA2... Read More about ALMA Reveals Strong [C II] Emission in a Galaxy Embedded in a Giant Lyα Blob at z = 3.1.

The Chandra Deep Field-South Survey: 7 Ms Source Catalogs (2016)
Journal Article
Luo, B., Brandt, W., Xue, Y., Lehmer, B., Alexander, D., Bauer, F., …Wang, J. (2017). The Chandra Deep Field-South Survey: 7 Ms Source Catalogs. Astrophysical Journal Supplement, 228(1), Article 2. https://doi.org/10.3847/1538-4365/228/1/2

We present X-ray source catalogs for the ≈7 Ms exposure of the Chandra Deep Field-South (CDF-S), which covers a total area of 484.2 arcmin2. Utilizing wavdetect for initial source detection and ACIS Extract for photometric extraction and significance... Read More about The Chandra Deep Field-South Survey: 7 Ms Source Catalogs.

Kiloparsec-scale Dust Disks in High-redshift Luminous Submillimeter Galaxies (2016)
Journal Article
Hodge, J., Swinbank, A., Simpson, J., Smail, I., Walter, F., Alexander, D., …van der Werf, P. (2016). Kiloparsec-scale Dust Disks in High-redshift Luminous Submillimeter Galaxies. Astrophysical Journal, 833(1), Article 103. https://doi.org/10.3847/1538-4357/833/1/103

We present high-resolution (0farcs16) 870 μm Atacama Large Millimeter/submillimeter Array (ALMA) imaging of 16 luminous (${L}_{\mathrm{IR}}\sim 4\times {10}^{12}\,{L}_{\odot }$) submillimeter galaxies (SMGs) from the ALESS survey of the Extended Chan... Read More about Kiloparsec-scale Dust Disks in High-redshift Luminous Submillimeter Galaxies.

ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: CO Luminosity Functions and the Evolution of the Cosmic Density of Molecular Gas (2016)
Journal Article
Decarli, R., Walter, F., Aravena, M., Carilli, C., Bouwens, R., da Cunha, E., …Wagg, J. (2016). ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: CO Luminosity Functions and the Evolution of the Cosmic Density of Molecular Gas. Astrophysical Journal, 833(1), Article 69. https://doi.org/10.3847/1538-4357/833/1/69

In this paper we use ASPECS, the ALMA Spectroscopic Survey in the Hubble Ultra Deep Field in band 3 and band 6, to place blind constraints on the CO luminosity function and the evolution of the cosmic molecular gas density as a function of redshift u... Read More about ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: CO Luminosity Functions and the Evolution of the Cosmic Density of Molecular Gas.

ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Survey Description (2016)
Journal Article
Walter, F., Decarli, R., Aravena, M., Carilli, C., Bouwens, R., da Cunha, E., …Wagg, J. (2016). ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Survey Description. Astrophysical Journal, 833(1), Article 67. https://doi.org/10.3847/1538-4357/833/1/67

We present the rationale for and the observational description of ASPECS: The ALMA SPECtroscopic Survey in the Hubble Ultra-Deep Field (UDF), the cosmological deep field that has the deepest multi-wavelength data available. Our overarching goal is to... Read More about ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Survey Description.

The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Search for [CII] Line and Dust Emission in 6 < z < 8 Galaxies (2016)
Journal Article
Aravena, M., Decarli, R., Walter, F., Bouwens, R., Oesch, P., Carilli, C., …Fudamoto, Y. (2016). The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Search for [CII] Line and Dust Emission in 6 < z < 8 Galaxies. Astrophysical Journal, 833(1), Article 71. https://doi.org/10.3847/1538-4357/833/1/71

We present a search for [C ii] line and dust continuum emission from optical dropout galaxies at z > 6 using ASPECS, our Atacama Large Millimeter submillimeter Array Spectroscopic Survey in the Hubble Ultra-deep Field (UDF). Our observations, which c... Read More about The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Search for [CII] Line and Dust Emission in 6 < z < 8 Galaxies.

The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Continuum Number Counts, Resolved 1.2 mm Extragalactic Background, and Properties of the Faintest Dusty Star-forming Galaxies (2016)
Journal Article
Aravena, M., Decarli, R., Walter, F., Da Cunha, E., Bauer, F., Carilli, C., …Wagg, J. (2016). The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Continuum Number Counts, Resolved 1.2 mm Extragalactic Background, and Properties of the Faintest Dusty Star-forming Galaxies. Astrophysical Journal, 833(1), Article 68. https://doi.org/10.3847/1538-4357/833/1/68

We present an analysis of a deep (1σ = 13 μJy) cosmological 1.2 mm continuum map based on ASPECS, the ALMA Spectroscopic Survey in the Hubble Ultra Deep Field. In the 1 arcmin2 covered by ASPECS we detect nine sources at \gt 3.5σ significance at 1.2... Read More about The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Continuum Number Counts, Resolved 1.2 mm Extragalactic Background, and Properties of the Faintest Dusty Star-forming Galaxies.

ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The Infrared Excess of UV-Selected z = 2-10 Galaxies as a Function of UV-Continuum Slope and Stellar Mass (2016)
Journal Article
Bouwens, R., Aravena, M., Decarli, R., Walter, F., da Cunha, E., Labbé, I., …Wilkins, S. (2016). ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The Infrared Excess of UV-Selected z = 2-10 Galaxies as a Function of UV-Continuum Slope and Stellar Mass. Astrophysical Journal, 833(1), Article 72. https://doi.org/10.3847/1538-4357/833/1/72

We make use of deep 1.2 mm continuum observations (12.7 μJy beam-1 rms) of a 1 arcmin2 region in the Hubble Ultra Deep Field to probe dust-enshrouded star formation from 330 Lyman-break galaxies spanning the redshift range z = 2-10 (to ˜2-3 M ⊙ yr-1... Read More about ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The Infrared Excess of UV-Selected z = 2-10 Galaxies as a Function of UV-Continuum Slope and Stellar Mass.

The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Molecular Gas Reservoirs in High-redshift Galaxies (2016)
Journal Article
Decarli, R., Walter, F., Aravena, M., Carilli, C., Bouwens, R., da Cunha, E., …van der Werf, P. (2016). The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Molecular Gas Reservoirs in High-redshift Galaxies. Astrophysical Journal, 833(1), Article 70. https://doi.org/10.3847/1538-4357/833/1/70

We study the molecular gas properties of high-z galaxies observed in the ALMA Spectroscopic Survey (ASPECS) that targets an ˜1 arcmin2 region in the Hubble Ultra Deep Field (UDF), a blind survey of CO emission (tracing molecular gas) in the 3 and 1 m... Read More about The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Molecular Gas Reservoirs in High-redshift Galaxies.

SINFONI-HiZELS: the dynamics, merger rates and metallicity gradients of `typical' star-forming galaxies at z = 0.8-2.2 (2016)
Journal Article
Molina, J., Ibar, E., Swinbank, A., Sobral, D., Best, P., Smail, I., …Cirasuolo, M. (2017). SINFONI-HiZELS: the dynamics, merger rates and metallicity gradients of `typical' star-forming galaxies at z = 0.8-2.2. Monthly Notices of the Royal Astronomical Society, 466(1), 892-905. https://doi.org/10.1093/mnras/stw3120

We present adaptive optics (AO) assisted SINFONI integral field unit (IFU) spectroscopy of 11 Hα emitting galaxies selected from the High-Z Emission Line Survey (HiZELS). We obtain spatially resolved dynamics on ∼kpc-scales of star-forming galaxies [... Read More about SINFONI-HiZELS: the dynamics, merger rates and metallicity gradients of `typical' star-forming galaxies at z = 0.8-2.2.

The CALYMHA survey: Lyα luminosity function and global escape fraction of Lyα photons at z = 2.23 (2016)
Journal Article
Sobral, D., Matthee, J., Best, P., Stroe, A., Röttgering, H., Oteo, I., …Paulino-Afonso, A. (2017). The CALYMHA survey: Lyα luminosity function and global escape fraction of Lyα photons at z = 2.23. Monthly Notices of the Royal Astronomical Society, 466(1), 1242-1258. https://doi.org/10.1093/mnras/stw3090

We present the CAlibrating LYMan-α with Hα (CALYMHA) pilot survey and new results on Lyman α (Lyα) selected galaxies at z ∼ 2. We use a custom-built Lyα narrow-band filter at the Isaac Newton Telescope, designed to provide a matched volume coverage t... Read More about The CALYMHA survey: Lyα luminosity function and global escape fraction of Lyα photons at z = 2.23.

The Space Density of Luminous Dusty Star-forming Galaxies at z > 4: SCUBA-2 and LABOCA Imaging of Ultrared Galaxies from Herschel-ATLAS (2016)
Journal Article
Ivison, R., Lewis, A., Weiss, A., Arumugam, V., Simpson, J., Holland, W., …Wardlow, J. (2016). The Space Density of Luminous Dusty Star-forming Galaxies at z > 4: SCUBA-2 and LABOCA Imaging of Ultrared Galaxies from Herschel-ATLAS. Astrophysical Journal, 832(1), Article 78. https://doi.org/10.3847/0004-637x/832/1/78

Until recently, only a handful of dusty, star-forming galaxies (DSFGs) were known at z > 4, most of them significantly amplified by gravitational lensing. Here, we have increased the number of such DSFGs substantially, selecting galaxies from the uni... Read More about The Space Density of Luminous Dusty Star-forming Galaxies at z > 4: SCUBA-2 and LABOCA Imaging of Ultrared Galaxies from Herschel-ATLAS.

The SCUBA-2 Cosmology Legacy Survey: 850 μm maps, catalogues and number counts (2016)
Journal Article
Geach, J., Dunlop, J., Halpern, M., Smail, I., van der Werf, P., Alexander, D., …Zemcov, M. (2017). The SCUBA-2 Cosmology Legacy Survey: 850 μm maps, catalogues and number counts. Monthly Notices of the Royal Astronomical Society, 465(2), 1789-1806. https://doi.org/10.1093/mnras/stw2721

We present a catalogue of ∼3000 submillimetre sources detected (≥3.5σ) at 850 μm over ∼5 deg2 surveyed as part of the James Clerk Maxwell Telescope (JCMT) SCUBA-2 Cosmology Legacy Survey (S2CLS). This is the largest survey of its kind at 850 μm, incr... Read More about The SCUBA-2 Cosmology Legacy Survey: 850 μm maps, catalogues and number counts.

Faint Submillimeter Galaxies Identified through Their Optical/Near-infrared Colors. I. Spatial Clustering and Halo Masses (2016)
Journal Article
Chen, C., Smail, I., Swinbank, A., Simpson, J., Almaini, O., Conselice, C., …Wilkinson, A. (2016). Faint Submillimeter Galaxies Identified through Their Optical/Near-infrared Colors. I. Spatial Clustering and Halo Masses. Astrophysical Journal, 831(1), Article 91. https://doi.org/10.3847/0004-637x/831/1/91

The properties of submillimeter galaxies (SMGs) that are fainter than the confusion limit of blank-field single-dish surveys (S850≲ 2 mJy) are poorly constrained. Using a newly developed color selection technique, Optical-Infrared Triple Color (OIRTC... Read More about Faint Submillimeter Galaxies Identified through Their Optical/Near-infrared Colors. I. Spatial Clustering and Halo Masses.

The SCUBA-2 Cosmology Legacy Survey: the clustering of submillimetre galaxies in the UKIDSS UDS field (2016)
Journal Article
Wilkinson, A., Almaini, O., Chen, C., Smail, I., Arumugam, V., Blain, A., …Wild, V. (2017). The SCUBA-2 Cosmology Legacy Survey: the clustering of submillimetre galaxies in the UKIDSS UDS field. Monthly Notices of the Royal Astronomical Society, 464(2), 1380-1392. https://doi.org/10.1093/mnras/stw2405

Submillimetre galaxies (SMGs) are among the most luminous dusty galaxies in the Universe, but their true nature remains unclear; are SMGs the progenitors of the massive elliptical galaxies we see in the local Universe, or are they just a short-lived... Read More about The SCUBA-2 Cosmology Legacy Survey: the clustering of submillimetre galaxies in the UKIDSS UDS field.

The growth of typical star-forming galaxies and their supermassive black holes across cosmic time since z~2 (2016)
Journal Article
Calhau, J., Sobral, D., Stroe, A., Best, P., Smail, I., Lehmer, B., …Thomson, A. (2017). The growth of typical star-forming galaxies and their supermassive black holes across cosmic time since z~2. Monthly Notices of the Royal Astronomical Society, 464(1), 303-311. https://doi.org/10.1093/mnras/stw2295

Understanding galaxy formation and evolution requires studying the interplay between the growth of galaxies and the growth of their black holes across cosmic time. Here, we explore a sample of Hα-selected star-forming galaxies from the High Redshift... Read More about The growth of typical star-forming galaxies and their supermassive black holes across cosmic time since z~2.

The nature of Hβ+[O III] and [O II] emitters to z ∼ 5 with HiZELS: stellar mass functions and the evolution of EWs (2016)
Journal Article
Khostovan, A., Sobral, D., Mobasher, B., Smail, I., Darvish, B., Nayyeri, H., …Stott, J. (2016). The nature of Hβ+[O III] and [O II] emitters to z ∼ 5 with HiZELS: stellar mass functions and the evolution of EWs. Monthly Notices of the Royal Astronomical Society, 463(3), 2363-2382. https://doi.org/10.1093/mnras/stw2174

We investigate the properties of ∼7000 narrow-band selected galaxies with strong Hβ+[O III] and [O II] nebular emission lines from the High-z Emission-Line Survey between z ∼ 0.8 and 5.0. Our sample covers a wide range in stellar mass (Mstellar ∼ 107... Read More about The nature of Hβ+[O III] and [O II] emitters to z ∼ 5 with HiZELS: stellar mass functions and the evolution of EWs.

Witnessing the Birth of the Red Sequence: ALMA High-resolution Imaging of [C II] and Dust in Two Interacting Ultra-red Starbursts at z = 4.425 (2016)
Journal Article
Oteo, I., Ivison, R., Dunne, L., Smail, I., Swinbank, A., Zhang, Z., …van Kampen, E. (2016). Witnessing the Birth of the Red Sequence: ALMA High-resolution Imaging of [C II] and Dust in Two Interacting Ultra-red Starbursts at z = 4.425. Astrophysical Journal, 827(1), Article 34. https://doi.org/10.3847/0004-637x/827/1/34

Exploiting the sensitivity and spatial resolution of the Atacama Large Millimeter/submillimeter Array, we have studied the morphology and the physical scale of the interstellar medium—both gas and dust—in SGP 38326, an unlensed pair of interacting st... Read More about Witnessing the Birth of the Red Sequence: ALMA High-resolution Imaging of [C II] and Dust in Two Interacting Ultra-red Starbursts at z = 4.425.

[O III] emission line as a tracer of star-forming galaxies at high redshifts: comparison between Hα and [O III] emitters at z=2.23 in HiZELS (2016)
Journal Article
Suzuki, T., Kodama, T., Sobral, D., Khostovan, A., Hayashi, M., Shimakawa, R., …Best, P. (2016). [O III] emission line as a tracer of star-forming galaxies at high redshifts: comparison between Hα and [O III] emitters at z=2.23 in HiZELS. Monthly Notices of the Royal Astronomical Society, 462(1), 181-189. https://doi.org/10.1093/mnras/stw1655

We investigate the properties of z = 2.23 Hα and [O III] λ5007 emitters using the narrow-band-selected samples obtained from the High-z Emission Line Survey. We construct two samples of the Hα and [O III] emitters and compare their integrated physica... Read More about [O III] emission line as a tracer of star-forming galaxies at high redshifts: comparison between Hα and [O III] emitters at z=2.23 in HiZELS.

ALMA observations of a z ≈ 3.1 protocluster: star formation from active galactic nuclei and Lyman-alpha blobs in an overdense environment (2016)
Journal Article
Alexander, D., Simpson, J., Harrison, C., Mullaney, J., Smail, I., Geach, J., …Yamada, T. (2016). ALMA observations of a z ≈ 3.1 protocluster: star formation from active galactic nuclei and Lyman-alpha blobs in an overdense environment. Monthly Notices of the Royal Astronomical Society, 461(3), 2944-2952. https://doi.org/10.1093/mnras/stw1509

We exploit Atacama Large Interferometer Array (ALMA) 870 μm observations to measure the star formation rates (SFRs) of eight X-ray detected active galactic nuclei (AGNs) in a z ≈ 3.1 protocluster, four of which reside in extended Lyα haloes (often te... Read More about ALMA observations of a z ≈ 3.1 protocluster: star formation from active galactic nuclei and Lyman-alpha blobs in an overdense environment.

Herschel protocluster survey: a search for dusty star-forming galaxies in protoclusters at z = 2–3 (2016)
Journal Article
Kato, Y., Matsuda, Y., Smail, I., Swinbank, A., Hatsukade, B., Umehata, H., …Hayashino, T. (2016). Herschel protocluster survey: a search for dusty star-forming galaxies in protoclusters at z = 2–3. Monthly Notices of the Royal Astronomical Society, 460(4), 3861-3872. https://doi.org/10.1093/mnras/stw1237

We present a Herschel/SPIRE survey of three protoclusters at z = 2 − 3 (2QZCluster, HS1700, SSA22). Based on the SPIRE colours (S350/S250 and S500/S350) of 250 μm sources, we selected high redshift dusty star-forming galaxies potentially associated w... Read More about Herschel protocluster survey: a search for dusty star-forming galaxies in protoclusters at z = 2–3.

ALMACAL I: First Dual-band Number Counts from a Deep and Wide ALMA Submillimeter Survey, Free from Cosmic Variance (2016)
Journal Article
Oteo, I., Zwaan, M., Ivison, R., Smail, I., & Biggs, A. (2016). ALMACAL I: First Dual-band Number Counts from a Deep and Wide ALMA Submillimeter Survey, Free from Cosmic Variance. Astrophysical Journal, 822(1), Article 36. https://doi.org/10.3847/0004-637x/822/1/36

We have exploited ALMA calibration observations to carry out a novel, wide, and deep submillimeter (submm) survey, almacal. These calibration data comprise a large number of observations of calibrator fields in a variety of frequency bands and array... Read More about ALMACAL I: First Dual-band Number Counts from a Deep and Wide ALMA Submillimeter Survey, Free from Cosmic Variance.

The Spatially Resolved Dynamics of Dusty Starburst Galaxies in a z ~ 0.4 Cluster: Beginning the Transition from Spirals to S0s (2016)
Journal Article
Johnson, H., Harrison, C., Swinbank, A., Bower, R., Smail, I., Koyama, Y., & Geach, J. (2016). The Spatially Resolved Dynamics of Dusty Starburst Galaxies in a z ~ 0.4 Cluster: Beginning the Transition from Spirals to S0s. Monthly Notices of the Royal Astronomical Society, 460(1), 1059-1076. https://doi.org/10.1093/mnras/stw1030

To investigate what drives the reversal of the morphology–density relation at intermediate/high redshift, we present a multiwavelength analysis of 27 dusty starburst galaxies in the massive cluster Cl 0024+17 at z = 0.4. We combine Hα dynamical maps... Read More about The Spatially Resolved Dynamics of Dusty Starburst Galaxies in a z ~ 0.4 Cluster: Beginning the Transition from Spirals to S0s.

The KMOS Redshift One Spectroscopic Survey (KROSS): the Tully–Fisher relation at z ∼ 1 (2016)
Journal Article
Tiley, A., Stott, J., Swinbank, A., Bureau, M., Harrison, C., Bower, R., …Best, P. (2016). The KMOS Redshift One Spectroscopic Survey (KROSS): the Tully–Fisher relation at z ∼ 1. Monthly Notices of the Royal Astronomical Society, 460(1), 103-129. https://doi.org/10.1093/mnras/stw936

We present the stellar mass (M*), and K-corrected K-band absolute magnitude (MK) Tully–Fisher relations (TFRs) for subsamples of the 584 galaxies spatially resolved in H α emission by the KMOS Redshift One Spectroscopic Survey (KROSS). We model the v... Read More about The KMOS Redshift One Spectroscopic Survey (KROSS): the Tully–Fisher relation at z ∼ 1.

A complete census of Herschel-detected infrared sources within the HST Frontier Fields (2016)
Journal Article
Rawle, T., Altieri, B., Egami, E., Pérez-González, P., Boone, F., Clement, B., …Smail, I. (2016). A complete census of Herschel-detected infrared sources within the HST Frontier Fields. Monthly Notices of the Royal Astronomical Society, 459(2), 1626-1645. https://doi.org/10.1093/mnras/stw712

We present a complete census of all Herschel-detected sources within the six massive lensing clusters of the HST Frontier Fields (HFF). We provide a robust legacy catalogue of 263 sources with Herschel fluxes, primarily based on imaging from the Hers... Read More about A complete census of Herschel-detected infrared sources within the HST Frontier Fields.

The SCUBA-2 Cosmology Legacy Survey: Multi-wavelengths counterparts to 10^3 submillimeter galaxies in the UKIDSS-UDS field (2016)
Journal Article
Chen, C., Smail, I., Ivison, R., Arumugam, V., Almaini, O., Conselice, C., …Zavala, J. (2016). The SCUBA-2 Cosmology Legacy Survey: Multi-wavelengths counterparts to 10^3 submillimeter galaxies in the UKIDSS-UDS field. Astrophysical Journal, 820(2), Article 82. https://doi.org/10.3847/0004-637x/820/2/82

We present multiwavelength identifications for the counterparts of 1088 submillimeter sources detected at 850 μm in the SCUBA-2 Cosmology Legacy Survey study of the UKIRT Infrared Deep Sky Survey-Ultra-Deep Survey (UDS) field. By utilizing an Atacama... Read More about The SCUBA-2 Cosmology Legacy Survey: Multi-wavelengths counterparts to 10^3 submillimeter galaxies in the UKIDSS-UDS field.

The CALYMHA survey: Lyα escape fraction and its dependence on galaxy properties at z = 2.23 (2016)
Journal Article
Matthee, J., Sobral, D., Oteo, I., Best, P., Smail, I., Röttgering, H., & Paulino-Afonso, A. (2016). The CALYMHA survey: Lyα escape fraction and its dependence on galaxy properties at z = 2.23. Monthly Notices of the Royal Astronomical Society, 458(1), 449-467. https://doi.org/10.1093/mnras/stw322

We present the first results from our CAlibrating LYMan-α with Hα (CALYMHA) pilot survey at the Isaac Newton Telescope. We measure Lyα emission for 488 Hα selected galaxies at z = 2.23 from HiZELS in the COSMOS and UDS fields with a specially designe... Read More about The CALYMHA survey: Lyα escape fraction and its dependence on galaxy properties at z = 2.23.

The KMOS Redshift One Spectroscopic Survey (KROSS): dynamical properties, gas and dark matter fractions of typical z~1 star-forming galaxies (2016)
Journal Article
Stott, J., Swinbank, A., Johnson, H., Tiley, A., Magdis, G., Bower, R., …Cirasuolo, M. (2016). The KMOS Redshift One Spectroscopic Survey (KROSS): dynamical properties, gas and dark matter fractions of typical z~1 star-forming galaxies. Monthly Notices of the Royal Astronomical Society, 457(2), 1888-1904. https://doi.org/10.1093/mnras/stw129

The KMOS Redshift One Spectroscopic Survey (KROSS) is an ESO-guaranteed time survey of 795 typical star-forming galaxies in the redshift range z = 0.8–1.0 with the KMOS instrument on the Very Large Telescope. In this paper, we present resolved kinema... Read More about The KMOS Redshift One Spectroscopic Survey (KROSS): dynamical properties, gas and dark matter fractions of typical z~1 star-forming galaxies.

The most luminous H α emitters at z ∼ 0.8–2.23 from HiZELS: evolution of AGN and star-forming galaxies (2016)
Journal Article
Sobral, D., Kohn, S., Best, P., Smail, I., Harrison, C., Stott, J., …Matthee, J. (2016). The most luminous H α emitters at z ∼ 0.8–2.23 from HiZELS: evolution of AGN and star-forming galaxies. Monthly Notices of the Royal Astronomical Society, 457(2), 1739-1752. https://doi.org/10.1093/mnras/stw022

We use new near-infrared spectroscopic observations to investigate the nature and evolution of the most luminous Hα emitters at z ∼ 0.8–2.23, which evolve strongly in number density over this period, and compare them to more typical Hα emitters. We s... Read More about The most luminous H α emitters at z ∼ 0.8–2.23 from HiZELS: evolution of AGN and star-forming galaxies.

ALMA resolves extended star formation in high-z AGN host galaxies (2016)
Journal Article
Harrison, C., Simpson, J., Stanley, F., Alexander, D., Daddi, E., Mullaney, J., …Smail, I. (2016). ALMA resolves extended star formation in high-z AGN host galaxies. Monthly Notices of the Royal Astronomical Society: Letters, 457(1), L122-L126. https://doi.org/10.1093/mnrasl/slw001

We present high-resolution (0.3 arcsec) Atacama Large Millimeter Array (ALMA) 870 μm imaging of five z ≈ 1.5–4.5 X-ray detected AGN (with luminosities of L2–8keV > 1042 erg s−1). These data provide a ≳20 times improvement in spatial resolution over s... Read More about ALMA resolves extended star formation in high-z AGN host galaxies.

ALMA Deep Field in SSA22: A Concentration of Dusty Starbursts in a z = 3.09 Protocluster Core (2015)
Journal Article
Umehata, H., Tamura, Y., Kohno, K., Ivison, R., Alexander, D., Geach, J., …Yun, M. (2015). ALMA Deep Field in SSA22: A Concentration of Dusty Starbursts in a z = 3.09 Protocluster Core. Astrophysical Journal Letters, 815, Article L8. https://doi.org/10.1088/2041-8205/815/1/l8

We report the results of 1farcm5 × 3' mapping at 1.1 mm with the Atacama Large Millimeter/submillimeter Array toward the central region of the z = 3.09 SSA22 protocluster. By combining our source catalog with archival spectroscopic redshifts, we find... Read More about ALMA Deep Field in SSA22: A Concentration of Dusty Starbursts in a z = 3.09 Protocluster Core.

A millimetre-wave redshift search for the unlensed HyLIRG, HS1700.850.1 (2015)
Journal Article
Chapman, S., Bertoldi, F., Smail, I., Steidel, C., Blain, A., Geach, J., …Reddy, N. (2015). A millimetre-wave redshift search for the unlensed HyLIRG, HS1700.850.1. Monthly Notices of the Royal Astronomical Society, 453(1), 951-959. https://doi.org/10.1093/mnras/stv1618

We report the redshift of an unlensed, highly obscured submillimetre galaxy (SMG), HS1700.850.1, the brightest SMG (S850 μm = 19.1 mJy) detected in the James Clerk Maxwell Telescope/Submillimetre Common-user Bolometer Array-2 (JCMT/SCUBA-2) Baryonic... Read More about A millimetre-wave redshift search for the unlensed HyLIRG, HS1700.850.1.

Evolution of the H β + [O III] and [O II] luminosity functions and the [O II] star formation history of the Universe up to z ∼ 5 from HiZELS (2015)
Journal Article
Khostovan, A., Sobral, D., Mobasher, B., Best, P., Smail, I., Stott, J., …Nayyeri, H. (2015). Evolution of the H β + [O III] and [O II] luminosity functions and the [O II] star formation history of the Universe up to z ∼ 5 from HiZELS. Monthly Notices of the Royal Astronomical Society, 452(4), 3948-3968. https://doi.org/10.1093/mnras/stv1474

We investigate the evolution of the H β + [O iii] and [O ii] luminosity functions from z ∼ 0.8 to ∼5 in four redshift slices per emission line using data from the High-z Emission Line Survey (HiZELS). This is the first time that the H β + [O iii] and... Read More about Evolution of the H β + [O III] and [O II] luminosity functions and the [O II] star formation history of the Universe up to z ∼ 5 from HiZELS.

Revealing the complex nature of the strong gravitationally lensed system H-ATLAS J090311.6+003906 using ALMA (2015)
Journal Article
Dye, S., Furlanetto, C., Swinbank, A., Vlahakis, C., Nightingale, J., Dunne, L., …van der Werf, P. (2015). Revealing the complex nature of the strong gravitationally lensed system H-ATLAS J090311.6+003906 using ALMA. Monthly Notices of the Royal Astronomical Society, 452(3), 2258-2268. https://doi.org/10.1093/mnras/stv1442

We have modelled Atacama Large Millimetre/sub-millimetre Array (ALMA) long baseline imaging of the strong gravitational lens system H-ATLAS J090311.6+003906 (SDP.81). We have reconstructed the distribution of band 6 and 7 continuum emission in the z... Read More about Revealing the complex nature of the strong gravitationally lensed system H-ATLAS J090311.6+003906 using ALMA.

On the nature of Hα emitters at z ∼ 2 from the HiZELS survey: physical properties, Lyα escape fraction and main sequence (2015)
Journal Article
Oteo, I., Sobral, D., Ivison, R., Smail, I., Best, P., Cepa, J., & Pérez-García, A. (2015). On the nature of Hα emitters at z ∼ 2 from the HiZELS survey: physical properties, Lyα escape fraction and main sequence. Monthly Notices of the Royal Astronomical Society, 452(2), 2018-2033. https://doi.org/10.1093/mnras/stv1284

We present a detailed multiwavelength study (from rest-frame ultraviolet to far-infrared) of narrow-band selected, star-forming (SF) Hα emitters (HAEs) at z ∼ 2.23 taken from the High-Redshift(Z) Emission Line Survey (HiZELS). We find that HAEs have... Read More about On the nature of Hα emitters at z ∼ 2 from the HiZELS survey: physical properties, Lyα escape fraction and main sequence.

Early Science with the Large Millimeter Telescope: observations of dust continuum and CO emission lines of cluster-lensed submillimetre galaxies at z=2.0-4.7 (2015)
Journal Article
Zavala, J., Yun, M., Aretxaga, I., Hughes, D., Wilson, G., Geach, J., …Zeballos, M. (2015). Early Science with the Large Millimeter Telescope: observations of dust continuum and CO emission lines of cluster-lensed submillimetre galaxies at z=2.0-4.7. Monthly Notices of the Royal Astronomical Society, 452(2), 1140-1151. https://doi.org/10.1093/mnras/stv1351

We present Early Science observations with the Large Millimeter Telescope, AzTEC 1.1 mm continuum images and wide bandwidth spectra (73–111 GHz) acquired with the Redshift Search Receiver, towards four bright lensed submillimetre galaxies identified... Read More about Early Science with the Large Millimeter Telescope: observations of dust continuum and CO emission lines of cluster-lensed submillimetre galaxies at z=2.0-4.7.

CF-HiZELS, an ∼10 deg2 emission-line survey with spectroscopic follow-up: Hα, [O iii] + Hβ and [O ii] luminosity functions at z = 0.8, 1.4 and 2.2 (2015)
Journal Article
Sobral, D., Matthee, J., Best, P., Smail, I., Khostovan, A., Milvang-Jensen, B., …Mobasher, B. (2015). CF-HiZELS, an ∼10 deg2 emission-line survey with spectroscopic follow-up: Hα, [O iii] + Hβ and [O ii] luminosity functions at z = 0.8, 1.4 and 2.2. Monthly Notices of the Royal Astronomical Society, 451(3), 2303-2323. https://doi.org/10.1093/mnras/stv1076

We present results from the largest contiguous narrow-band survey in the near-infrared. We have used the wide-field infrared camera/Canada–France–Hawaii Telescope and the lowOH2 filter (1.187 ± 0.005 μm) to survey ≈10 deg2 of contiguous extragalactic... Read More about CF-HiZELS, an ∼10 deg2 emission-line survey with spectroscopic follow-up: Hα, [O iii] + Hβ and [O ii] luminosity functions at z = 0.8, 1.4 and 2.2.

The SCUBA-2 Cosmology Legacy Survey: ALMA resolves the bright-end of the submillimeter number counts (2015)
Journal Article
Simpson, J., Smail, I., Swinbank, A., Chapman, S., Geach, J., Ivison, R., …van der Werf, P. (2015). The SCUBA-2 Cosmology Legacy Survey: ALMA resolves the bright-end of the submillimeter number counts. Astrophysical Journal, 807(2), Article 128. https://doi.org/10.1088/0004-637x/807/2/128

We present high-resolution 870 μm Atacama Large Millimeter/sub-millimeter Array (ALMA) continuum maps of 30 bright sub-millimeter sources in the UKIDSS UDS field. These sources are selected from deep, 1 degree2 850 μm maps from the SCUBA-2 Cosmology... Read More about The SCUBA-2 Cosmology Legacy Survey: ALMA resolves the bright-end of the submillimeter number counts.

Dusty starbursts and the formation of elliptical galaxies: A SCUBA-2 survey of a z = 1.46 cluster (2015)
Journal Article
Ma, C., Smail, I., Swinbank, A., Simpson, J., Thomson, A., Chen, C., …Kodama, T. (2015). Dusty starbursts and the formation of elliptical galaxies: A SCUBA-2 survey of a z = 1.46 cluster. Astrophysical Journal, 806(2), Article 257. https://doi.org/10.1088/0004-637x/806/2/257

We report the results of a deep SCUBA-2 850 and 450 μm survey for dust-obscured ultra-/luminous infrared galaxies (U/LIRGs) in the field of the z = 1.46 cluster XCS J2215.9−1738. We detect a striking overdensity of submillimeter sources coincident wi... Read More about Dusty starbursts and the formation of elliptical galaxies: A SCUBA-2 survey of a z = 1.46 cluster.

An ALMA Survey of Sub-millimeter Galaxies in the Extended Chandra Deep Field South: Physical Properties Derived from Ultraviolet-to-radio Modeling (2015)
Journal Article
da Cunha, E., Walter, F., Smail, I., Swinbank, A., Simpson, J., Decarli, R., …Thomson, A. (2015). An ALMA Survey of Sub-millimeter Galaxies in the Extended Chandra Deep Field South: Physical Properties Derived from Ultraviolet-to-radio Modeling. Astrophysical Journal, 806(1), https://doi.org/10.1088/0004-637x/806/1/110

The ALESS survey has followed up on a sample of 122 sub-millimeter sources in the Extended Chandra Deep Field South at 870 μmwith the Atacama Large Millimeter Array (ALMA), allowing us to pinpoint the positions of submillimeter galaxies (SMGs) to ∼0.... Read More about An ALMA Survey of Sub-millimeter Galaxies in the Extended Chandra Deep Field South: Physical Properties Derived from Ultraviolet-to-radio Modeling.

Resolved spectroscopy of gravitationally lensed galaxies: global dynamics and star-forming clumps on ∼100 pc scales at 1 < z < 4 (2015)
Journal Article
Livermore, R., Jones, T., Richard, J., Bower, R., Swinbank, A., Yuan, T., …Ebeling, H. (2015). Resolved spectroscopy of gravitationally lensed galaxies: global dynamics and star-forming clumps on ∼100 pc scales at 1 < z < 4. Monthly Notices of the Royal Astronomical Society, 450(2), 1812-1835. https://doi.org/10.1093/mnras/stv686

We present adaptive optics-assisted integral field spectroscopy around the Hα or Hβ lines of 12 gravitationally lensed galaxies obtained with VLT/SINFONI, Keck/OSIRIS and Gemini/NIFS. We combine these data with previous observations and investigate t... Read More about Resolved spectroscopy of gravitationally lensed galaxies: global dynamics and star-forming clumps on ∼100 pc scales at 1 < z < 4.

ALMA Resolves the Properties of Star-forming Regions in a Dense Gas Disk at z ~ 3 (2015)
Journal Article
Swinbank, A., Dye, S., Nightingale, J., Furlanetto, C., Smail, I., Cooray, A., …Vlahakis, C. (2015). ALMA Resolves the Properties of Star-forming Regions in a Dense Gas Disk at z ~ 3. Astrophysical Journal Letters, 806(1), Article L17. https://doi.org/10.1088/2041-8205/806/1/l17

We exploit long baseline ALMA submillimeter observations of the lensed star-forming galaxy SDP 81 at z = 3.042 to investigate the properties of the interstellar medium (ISM) on scales of 50–100 pc. The kinematics of the 12CO gas within this system ar... Read More about ALMA Resolves the Properties of Star-forming Regions in a Dense Gas Disk at z ~ 3.

GLACE survey: OSIRIS/GTC tuneable filter Hα imaging of the rich galaxy cluster ZwCl 0024.0+1652 at z = 0.395. I. Survey presentation, TF data reduction techniques, and catalogue (2015)
Journal Article
Sánchez-Portal, M., Pintos-Castro, I., Pérez-Martínez, R., Cepa, J., Pérez García, A., Domínguez-Sánchez, H., …Valtchanov, I. (2015). GLACE survey: OSIRIS/GTC tuneable filter Hα imaging of the rich galaxy cluster ZwCl 0024.0+1652 at z = 0.395. I. Survey presentation, TF data reduction techniques, and catalogue. Astronomy & Astrophysics, 578, Article A30. https://doi.org/10.1051/0004-6361/201525620

The cores of clusters at 0 ≲ z ≲ 1 are dominated by quiescent early-type galaxies, whereas the field is dominated by star-forming late-type galaxies. Clusters grow through the accretion of galaxies and groups from the surrounding field, which implies... Read More about GLACE survey: OSIRIS/GTC tuneable filter Hα imaging of the rich galaxy cluster ZwCl 0024.0+1652 at z = 0.395. I. Survey presentation, TF data reduction techniques, and catalogue.

Mapping the dynamics of a giant Ly alpha halo at z = 4.1 with MUSE: the energetics of a large-scale AGN-driven outflow around a massive, high-redshift galaxy (2015)
Journal Article
Swinbank, A., Vernet, J., Smail, I., De Breuck, C., Bacon, R., Contini, T., …Venemans, B. (2015). Mapping the dynamics of a giant Ly alpha halo at z = 4.1 with MUSE: the energetics of a large-scale AGN-driven outflow around a massive, high-redshift galaxy. Monthly Notices of the Royal Astronomical Society, 449(2), 1298-1308. https://doi.org/10.1093/mnras/stv366

We present Multi Unit Spectroscopic Explorer (MUSE) integral field unit spectroscopic observations of the ∼150 kpc Lyα halo around the z = 4.1 radio galaxy TN J1338−1942. This 9-h observation maps the full two-dimensional kinematics of the Lyα emissi... Read More about Mapping the dynamics of a giant Ly alpha halo at z = 4.1 with MUSE: the energetics of a large-scale AGN-driven outflow around a massive, high-redshift galaxy.

A blind CO detection of a distant red galaxy in the HS1700+64 protocluster (2015)
Journal Article
Chapman, S., Bertoldi, F., Smail, I., Blain, A., Geach, J., Gurwell, M., …Steidel, C. (2015). A blind CO detection of a distant red galaxy in the HS1700+64 protocluster. Monthly Notices of the Royal Astronomical Society: Letters, 449(1), L68-L72. https://doi.org/10.1093/mnrasl/slv010

We report the blind detection of 12CO emission from a distant red galaxy, HS1700.DRG55. We have used the IRAM Plateau de Bure Interferometer WideX, with its 3.6 GHz of instantaneous dual-polarization bandwidth, to target 12CO(3–2) from galaxies lying... Read More about A blind CO detection of a distant red galaxy in the HS1700+64 protocluster.

Tracing cool molecular gas and star formation on ∼100 pc scales within a z ∼ 2.3 galaxy (2015)
Journal Article
Thomson, A., Ivison, R., Owen, F. N., Danielson, A., Swinbank, A., & Smail, I. (2015). Tracing cool molecular gas and star formation on ∼100 pc scales within a z ∼ 2.3 galaxy. Monthly Notices of the Royal Astronomical Society, 448(2), 1874-1886. https://doi.org/10.1093/mnras/stv118

We present new, high-angular resolution interferometric observations with the Karl G. Jansky Very Large Array of 12CO J = 1−0 line emission and 4–8 GHz continuum emission in the strongly lensed, z = 2.3 submillimetre galaxy, SMM J21352-0102. Using th... Read More about Tracing cool molecular gas and star formation on ∼100 pc scales within a z ∼ 2.3 galaxy.

COLDz: Karl G. Jansky Very Large Array Discovery of a Gas-rich Galaxy in COSMOS (2015)
Journal Article
Lentati, L., Wagg, J., Carilli, C., Riechers, D., Capak, P., Walter, F., …Smolčć, V. (2015). COLDz: Karl G. Jansky Very Large Array Discovery of a Gas-rich Galaxy in COSMOS. Astrophysical Journal, 800(1), Article 67. https://doi.org/10.1088/0004-637x/800/1/67

The broad spectral bandwidth at millimeter and centimeter wavelengths provided by the recent upgrades to the Karl G. Jansky Very Large Array (VLA) has made it possible to conduct unbiased searches for molecular CO line emission at redshifts, z > 1.31... Read More about COLDz: Karl G. Jansky Very Large Array Discovery of a Gas-rich Galaxy in COSMOS.

An ALMA Survey of Submillimeter Galaxies in the Extended Chandra Deep Field South: Near-infrared Morphologies and Stellar Sizes (2015)
Journal Article
Chen, C., Smail, I., Swinbank, A., Simpson, J., Ma, C., Alexander, D., …van der Werf, P. (2015). An ALMA Survey of Submillimeter Galaxies in the Extended Chandra Deep Field South: Near-infrared Morphologies and Stellar Sizes. Astrophysical Journal, 799(2), Article 194. https://doi.org/10.1088/0004-637x/799/2/194

We analyze Hubble Space Telescope WFC3/H 160-band observations of a sample of 48 Atacama Large Millimeter/submillimeter Array detected submillimeter galaxies (SMGs) in the Extended Chandra Deep Field South field, to study their stellar morphologies a... Read More about An ALMA Survey of Submillimeter Galaxies in the Extended Chandra Deep Field South: Near-infrared Morphologies and Stellar Sizes.

The SCUBA-2 Cosmology Legacy Survey: ALMA Resolves the Rest-frame Far-infrared Emission of Sub-millimeter Galaxies (2015)
Journal Article
Simpson, J., Smail, I., Swinbank, A., Almaini, O., Blain, A., Bremer, M., …van der Werf, P. (2015). The SCUBA-2 Cosmology Legacy Survey: ALMA Resolves the Rest-frame Far-infrared Emission of Sub-millimeter Galaxies. Astrophysical Journal, 799(1), Article 81. https://doi.org/10.1088/0004-637x/799/1/81

We present high-resolution (0.''3) Atacama Large Millimeter Array 870 μm imaging of 52 sub-millimeter galaxies (SMGs) in the Ultra Deep Survey field to investigate the size and morphology of the sub-millimeter (sub-mm) emission on 2-10 kpc scales. We... Read More about The SCUBA-2 Cosmology Legacy Survey: ALMA Resolves the Rest-frame Far-infrared Emission of Sub-millimeter Galaxies.

The environments of Ly α blobs I: Wide-field Ly α imaging of TN J1338-1942, a powerful radio galaxy at z ≃ 4.1 associated with a giant Ly α nebula (2015)
Journal Article
Saito, T., Matsuda, Y., Lacey, C., Smail, I., Orsi, A., Baugh, C., …Taniguchi, Y. (2015). The environments of Ly α blobs I: Wide-field Ly α imaging of TN J1338-1942, a powerful radio galaxy at z ≃ 4.1 associated with a giant Ly α nebula. Monthly Notices of the Royal Astronomical Society, 447(4), 3069-3086. https://doi.org/10.1093/mnras/stu2538

We exploit wide-field Ly α imaging with Subaru to probe the environment around TN J1338−1942, a powerful radio galaxy with a > 100 kpc Ly α halo at z = 4.11. We used a sample of Ly α emitters (LAEs) down to log (LLyα[ erg s−1]) ∼ 42.8 to measure the... Read More about The environments of Ly α blobs I: Wide-field Ly α imaging of TN J1338-1942, a powerful radio galaxy at z ≃ 4.1 associated with a giant Ly α nebula.

Disentangling a group of lensed submm galaxies at z∼ 2.9 (2014)
Journal Article
MacKenzie, T., Scott, D., Smail, I., Chapin, E., Chapman, S., Conley, A., …Wardlow, J. (2014). Disentangling a group of lensed submm galaxies at z∼ 2.9. Monthly Notices of the Royal Astronomical Society, 445(1), 201-212. https://doi.org/10.1093/mnras/stu1623

MS 0451.6−0305 is a rich galaxy cluster whose strong lensing is particularly prominent at submm wavelengths. We combine new Submillimetre Common-User Bolometer Array (SCUBA)-2 data with imaging from Herschel Spectral and Photometric Imaging Receiver... Read More about Disentangling a group of lensed submm galaxies at z∼ 2.9.

Cosmic Web and Star Formation Activity in Galaxies at z ~ 1 (2014)
Journal Article
Darvish, B., Sobral, D., Mobasher, B., Scoville, N., Best, P., Sales, L., & Smail, I. (2014). Cosmic Web and Star Formation Activity in Galaxies at z ~ 1. Astrophysical Journal, 796(1), Article 51. https://doi.org/10.1088/0004-637x/796/1/51

We investigate the role of the delineated cosmic web/filaments on star formation activity by exploring a sample of 425 narrow-band selected Hα emitters, as well as 2846 color-color selected underlying star-forming galaxies for a large-scale structure... Read More about Cosmic Web and Star Formation Activity in Galaxies at z ~ 1.

Imaging the Environment of a z = 6.3 Submillimeter Galaxy with SCUBA-2 (2014)
Journal Article
Robson, E., Ivison, R., Smail, I., Holland, W., Geach, J., Gibb, A., …Wardlow, J. (2014). Imaging the Environment of a z = 6.3 Submillimeter Galaxy with SCUBA-2. Astrophysical Journal, 793(1), Article 11. https://doi.org/10.1088/0004-637x/793/1/11

We describe a search for submillimeter emission in the vicinity of one of the most distant, luminous galaxies known, HerMES FLS3, at z = 6.34, exploiting it as a signpost to a potentially biased region of the early universe, as might be expected in h... Read More about Imaging the Environment of a z = 6.3 Submillimeter Galaxy with SCUBA-2.

Detection of molecular gas in an ALMA [C II]-identified submillimetre galaxy at z = 4.44 (2014)
Journal Article
Huynh, M., Kimball, A., Norris, R., Smail, I., Chow, K., Coppin, K., …Swinbank, A. (2014). Detection of molecular gas in an ALMA [C II]-identified submillimetre galaxy at z = 4.44. Monthly Notices of the Royal Astronomical Society: Letters, 443(1), L54-L58. https://doi.org/10.1093/mnrasl/slu077

We present the detection of 12CO(2–1) in the z = 4.44 submillimetre galaxy ALESS65.1 using the Australia Telescope Compact Array. A previous Atacama Large Millimeter/submillimeter Array study of submillimetre galaxies (SMGs) in the Extended Chandra D... Read More about Detection of molecular gas in an ALMA [C II]-identified submillimetre galaxy at z = 4.44.

A relationship between specific star formation rate and metallicity gradient within z ∼ 1 galaxies from KMOS-HiZELS (2014)
Journal Article
Stott, J., Sobral, D., Swinbank, A., Smail, I., Bower, R., Best, P., …Matthee, J. (2014). A relationship between specific star formation rate and metallicity gradient within z ∼ 1 galaxies from KMOS-HiZELS. Monthly Notices of the Royal Astronomical Society, 443(3), 2695-2704. https://doi.org/10.1093/mnras/stu1343

We have observed a sample of typical z ∼ 1 star-forming galaxies, selected from the HiZELS survey, with the new K-band Multi-Object Spectrograph (KMOS) near-infrared, multi-integral field unit instrument on the Very Large Telescope (VLT), in order to... Read More about A relationship between specific star formation rate and metallicity gradient within z ∼ 1 galaxies from KMOS-HiZELS.

Herschel reveals a molecular outflow in a z = 2.3 ULIRG (2014)
Journal Article
George, R., Ivison, R., Smail, I., Swinbank, A., Hopwood, R., Stanley, F., …Werf, P. V. D. (2014). Herschel reveals a molecular outflow in a z = 2.3 ULIRG. Monthly Notices of the Royal Astronomical Society, 442(2), 1877-1883. https://doi.org/10.1093/mnras/stu967

We report the results from a 19-h integration with the Spectral and Photometric Imaging REceiver (SPIRE) Fourier Transform Spectrometer aboard the Herschel Space Observatory which has revealed the presence of a molecular outflow from the Cosmic Eyela... Read More about Herschel reveals a molecular outflow in a z = 2.3 ULIRG.

An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field South: radio properties and the far-infrared/radio correlation (2014)
Journal Article
Thomson, A., Ivison, R., Simpson, J., Swinbank, A., Smail, I., Arumugam, V., …van der Werf, P. (2014). An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field South: radio properties and the far-infrared/radio correlation. Monthly Notices of the Royal Astronomical Society, 442(1), 577-588. https://doi.org/10.1093/mnras/stu839

We present a study of the radio properties of 870 μm-selected submillimetre galaxies (SMGs), observed at high resolution with Atacama Large Millimeter Array (ALMA) in the Extended Chandra Deep Field South. From our initial sample of 76 ALMA SMGs, we... Read More about An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field South: radio properties and the far-infrared/radio correlation.

Herschel-ATLAS: properties of dusty massive galaxies at low and high redshifts (2014)
Journal Article
Rowlands, K., Dunne, L., Dye, S., Aragón-Salamanca, A., Maddox, S., da Cunha, E., …Valiante, E. (2014). Herschel-ATLAS: properties of dusty massive galaxies at low and high redshifts. Monthly Notices of the Royal Astronomical Society, 441(2), 1017-1039. https://doi.org/10.1093/mnras/stu510

We present a comparison of the physical properties of a rest-frame 250-μm-selected sample of massive, dusty galaxies from 0 < z < 5.3. Our sample comprises 29 high-redshift submillimetre galaxies (SMGs) from the literature and 843 dusty galaxies at z... Read More about Herschel-ATLAS: properties of dusty massive galaxies at low and high redshifts.

An ALMA Survey of Submillimeter Galaxies in the Extended Chandra Deep Field South: The Redshift Distribution and Evolution of Submillimeter Galaxies (2014)
Journal Article
Simpson, J., Swinbank, A., Smail, I., Alexander, D., Brandt, W., Bertoldi, F., …van der Werf, P. (2014). An ALMA Survey of Submillimeter Galaxies in the Extended Chandra Deep Field South: The Redshift Distribution and Evolution of Submillimeter Galaxies. Astrophysical Journal, 788(2), https://doi.org/10.1088/0004-637x/788/2/125

We present the first photometric redshift distribution for a large sample of 870 μm submillimeter galaxies (SMGs) with robust identifications based on observations with ALMA. In our analysis we consider 96 SMGs in the Extended Chandra Deep Field Sout... Read More about An ALMA Survey of Submillimeter Galaxies in the Extended Chandra Deep Field South: The Redshift Distribution and Evolution of Submillimeter Galaxies.

ALMA resolves turbulent, rotating [CII] emission in a young starburst galaxy at z = 4.8 (2014)
Journal Article
De Breuck, C., Williams, R., Swinbank, M., Caselli, P., Coppin, K., Davis, T., …Zwaan, M. (2014). ALMA resolves turbulent, rotating [CII] emission in a young starburst galaxy at z = 4.8. Astronomy & Astrophysics, 565, https://doi.org/10.1051/0004-6361/201323331

We present spatially resolved Atacama Large Millimeter/submillimeter Array (ALMA) [Cii] observations of the z = 4.7555 submillimetre galaxy, ALESS 73.1. Our 0.̋5 FWHM map resolves the [Cii] emitting gas which is centred close to the active galactic n... Read More about ALMA resolves turbulent, rotating [CII] emission in a young starburst galaxy at z = 4.8.

A 10 deg^2 Lyman α survey at z=8.8 with spectroscopic follow-up: strong constraints on the luminosity function and implications for other surveys (2014)
Journal Article
Matthee, J., Sobral, D., Swinbank, A., Smail, I., Best, P., Kim, J., …Fynbo, J. (2014). A 10 deg^2 Lyman α survey at z=8.8 with spectroscopic follow-up: strong constraints on the luminosity function and implications for other surveys. Monthly Notices of the Royal Astronomical Society, 440(3), 2375-2387. https://doi.org/10.1093/mnras/stu392

Candidate galaxies at redshifts of z ∼ 10 are now being found in extremely deep surveys, probing very small areas. As a consequence, candidates are very faint, making spectroscopic confirmation practically impossible. In order to overcome such limita... Read More about A 10 deg^2 Lyman α survey at z=8.8 with spectroscopic follow-up: strong constraints on the luminosity function and implications for other surveys.

Mapping the large-scale structure around a z = 1.46 galaxy cluster in 3D using two adjacent narrow-band filters (2014)
Journal Article
Hayashi, M., Kodama, T., Koyama, Y., Tadaki, K., Tanaka, I., Shimakawa, R., …Smail, I. (2014). Mapping the large-scale structure around a z = 1.46 galaxy cluster in 3D using two adjacent narrow-band filters. Monthly Notices of the Royal Astronomical Society, 439(3), 2571-2583. https://doi.org/10.1093/mnras/stu115

We present a novel method to estimate accurate redshifts of star-forming galaxies by measuring the flux ratio of the same emission line observed through two adjacent narrow-band filters. We apply this method to our NB912 and new NB921 data taken with... Read More about Mapping the large-scale structure around a z = 1.46 galaxy cluster in 3D using two adjacent narrow-band filters.

[C II] and ^12CO(1-0) Emission Maps in HLSJ091828.6+514223: A Strongly Lensed Interacting System at z = 5.24 (2014)
Journal Article
Rawle, T., Egami, E., Bussmann, R., Gurwell, M., Ivison, R., Boone, F., …Zemcov, M. (2014). [C II] and ^12CO(1-0) Emission Maps in HLSJ091828.6+514223: A Strongly Lensed Interacting System at z = 5.24. Astrophysical Journal, 783(1), Article 59. https://doi.org/10.1088/0004-637x/783/1/59

We present Submillimeter Array [C II] 158 μm and Karl G. Jansky Very Large Array 12CO(1-0) line emission maps for the bright, lensed, submillimeter source at z = 5.2430 behind A 773: HLSJ091828.6+514223 (HLS0918). We combine these measurements with p... Read More about [C II] and ^12CO(1-0) Emission Maps in HLSJ091828.6+514223: A Strongly Lensed Interacting System at z = 5.24.

The SCUBA-2 Cosmology Legacy Survey: Ultraluminous star-forming galaxies in a z=1.6 cluster (2014)
Journal Article
Smail, I., Geach, J., Swinbank, A., Tadaki, K., Arumugam, V., Hartley, W., …Webb, T. (2014). The SCUBA-2 Cosmology Legacy Survey: Ultraluminous star-forming galaxies in a z=1.6 cluster. Astrophysical Journal, 782(1), Article 19. https://doi.org/10.1088/0004-637x/782/1/19

We analyze new SCUBA-2 submillimeter and archival SPIRE far-infrared imaging of a z = 1.62 cluster, Cl 0218.3–0510, which lies in the UKIRT Infrared Deep Sky Survey/Ultra-Deep Survey field of the SCUBA-2 Cosmology Legacy Survey. Combining these trace... Read More about The SCUBA-2 Cosmology Legacy Survey: Ultraluminous star-forming galaxies in a z=1.6 cluster.

The stellar mass function of star-forming galaxies and the mass-dependent SFR function since z = 2.23 from HiZELS (2014)
Journal Article
Sobral, D., Best, P., Smail, I., Mobasher, B., Stott, J., & Nisbet, D. (2014). The stellar mass function of star-forming galaxies and the mass-dependent SFR function since z = 2.23 from HiZELS. Monthly Notices of the Royal Astronomical Society, 437(4), 3516-3528. https://doi.org/10.1093/mnras/stt2159

We explore a large uniformly selected sample of Hα selected star-forming galaxies (SFGs) at z = 0.40, 0.84, 1.47, 2.23 to unveil the evolution of the star formation rate (SFR) function and the stellar mass function. We find strong evolution in the SF... Read More about The stellar mass function of star-forming galaxies and the mass-dependent SFR function since z = 2.23 from HiZELS.

An ALMA Survey of Sub-millimeter Galaxies in the Extended Chandra Deep Field South: Sub-millimeter Properties of Color-selected Galaxies (2014)
Journal Article
Decarli, R., Smail, I., Walter, F., Swinbank, A., Chapman, S., Coppin, K., …Weiß, A. (2014). An ALMA Survey of Sub-millimeter Galaxies in the Extended Chandra Deep Field South: Sub-millimeter Properties of Color-selected Galaxies. Astrophysical Journal, 780(2), Article 115. https://doi.org/10.1088/0004-637x/780/2/115

We study the sub-millimeter properties of color-selected galaxies via a stacking analysis applied for the first time to interferometric data at sub-millimeter wavelengths. We base our study on 344 GHz ALMA continuum observations of ~20''-wide fields... Read More about An ALMA Survey of Sub-millimeter Galaxies in the Extended Chandra Deep Field South: Sub-millimeter Properties of Color-selected Galaxies.

Star formation histories, extinction, and dust properties of strongly lensed z ~ 1.5-3 star-forming galaxies from the Herschel Lensing Survey (2014)
Journal Article
Sklias, P., Zamojski, M., Schaerer, D., Dessauges-Zavadsky, M., Egami, E., Rex, M., …Kneib, J. (2014). Star formation histories, extinction, and dust properties of strongly lensed z ~ 1.5-3 star-forming galaxies from the Herschel Lensing Survey. Astronomy & Astrophysics, 561, Article A149. https://doi.org/10.1051/0004-6361/201322424

Context. Multi-wavelength, optical to IR/submm observations of strongly lensed galaxies identified by the Herschel Lensing Survey are used to determine the physical properties of high-redshift star-forming galaxies close to or below the detection lim... Read More about Star formation histories, extinction, and dust properties of strongly lensed z ~ 1.5-3 star-forming galaxies from the Herschel Lensing Survey.

The dynamics of z = 0.8 Hα-selected star-forming galaxies from KMOS/CF-HiZELS (2013)
Journal Article
Sobral, D., Swinbank, A., Stott, J., Matthee, J., Bower, R., Smail, I., …Sharples, R. (2013). The dynamics of z = 0.8 Hα-selected star-forming galaxies from KMOS/CF-HiZELS. Astrophysical Journal, 779(2), Article 139. https://doi.org/10.1088/0004-637x/779/2/139

We present the spatially resolved Hα dynamics of 16 star-forming galaxies at z ~ 0.81 using the new KMOS multi-object integral field spectrograph on the ESO Very Large Telescope. These galaxies, selected using 1.18 μm narrowband imaging from the 10 d... Read More about The dynamics of z = 0.8 Hα-selected star-forming galaxies from KMOS/CF-HiZELS.

An ALMA survey of sub-millimetre Galaxies in the Extended Chandra Deep Field South: the far-infrared properties of SMGs (2013)
Journal Article
Swinbank, A., Simpson, J., Smail, I., Harrison, C., Hodge, J., Karim, A., …van der Werf, P. (2014). An ALMA survey of sub-millimetre Galaxies in the Extended Chandra Deep Field South: the far-infrared properties of SMGs. Monthly Notices of the Royal Astronomical Society, 438(2), 1267-1287. https://doi.org/10.1093/mnras/stt2273

We exploit Atacama Large Millimeter Array (ALMA) 870 μm observations of sub-millimetre sources in the Extended Chandra Deep Field South to investigate the far-infrared properties of high-redshift sub-millimetre galaxies (SMGs). Using the precisely lo... Read More about An ALMA survey of sub-millimetre Galaxies in the Extended Chandra Deep Field South: the far-infrared properties of SMGs.

A fundamental metallicity relation for galaxies at z = 0.84-1.47 from HiZELS (2013)
Journal Article
Stott, J., Sobral, D., Bower, R., Smail, I., Best, P., Matsuda, Y., …Kodama, T. (2013). A fundamental metallicity relation for galaxies at z = 0.84-1.47 from HiZELS. Monthly Notices of the Royal Astronomical Society, 436(2), 1130-1141. https://doi.org/10.1093/mnras/stt1641

We obtained Subaru FMOS observations of Hα emitting galaxies selected from the HiZELS, to investigate the relationship between stellar mass, metallicity and star formation rate (SFR) at z = 0.84–1.47, for comparison with the fundamental metallicity r... Read More about A fundamental metallicity relation for galaxies at z = 0.84-1.47 from HiZELS.

13CO and C18O emission from a dense gas disc at z = 2.3: abundance variations, cosmic rays and the initial conditions for star formation (2013)
Journal Article
Danielson, A., Swinbank, A., Smail, I., Bayet, E., van der Werf, P. P., Cox, P., …Ivison, R. (2013). 13CO and C18O emission from a dense gas disc at z = 2.3: abundance variations, cosmic rays and the initial conditions for star formation. Monthly Notices of the Royal Astronomical Society, 436(3), 2793-2809. https://doi.org/10.1093/mnras/stt1775

We analyse the spectral line energy distributions of 13CO and C18O for the J = 1→0 up to J = 7→6 transitions in the gravitationally lensed ultraluminous infrared galaxy SMM J2135−0102 at z = 2.3. This is the first detection of 13CO and C18O in a high... Read More about 13CO and C18O emission from a dense gas disc at z = 2.3: abundance variations, cosmic rays and the initial conditions for star formation.

Detection of Hα emission from z > 3.5 submillimetre luminous galaxies with AKARI-FUHYU spectroscopy (2013)
Journal Article
Sedgwick, C., Serjeant, S., Pearson, C., Smail, I., Im, M., Oyabu, S., …White, G. (2013). Detection of Hα emission from z > 3.5 submillimetre luminous galaxies with AKARI-FUHYU spectroscopy. Monthly Notices of the Royal Astronomical Society, 436(1), 395-400. https://doi.org/10.1093/mnras/stt1572

We present tentative Hα emission line detections of four submillimetre-detected galaxies at z > 3.5: the radio galaxies 8C1909+722 and 4C60.07 at signal-to-noise ratios (SNRs) of 3.1 and 2.5, and two submillimetre-selected galaxies (SMGs) near the fi... Read More about Detection of Hα emission from z > 3.5 submillimetre luminous galaxies with AKARI-FUHYU spectroscopy.

An ALMA Survey of Submillimeter Galaxies in the Extended Chandra Deep Field-South: The AGN Fraction and X-Ray Properties of Submillimeter Galaxies (2013)
Journal Article
Wang, S., Brandt, W., Luo, B., Smail, I., Alexander, D., Danielson, A., …van der Werf, P. (2013). An ALMA Survey of Submillimeter Galaxies in the Extended Chandra Deep Field-South: The AGN Fraction and X-Ray Properties of Submillimeter Galaxies. Astrophysical Journal, 778(2), Article 179. https://doi.org/10.1088/0004-637x/778/2/179

The large gas and dust reservoirs of submillimeter galaxies (SMGs) could potentially provide ample fuel to trigger an active galactic nucleus (AGN), but previous studies of the AGN fraction in SMGs have been controversial largely due to the inhomogen... Read More about An ALMA Survey of Submillimeter Galaxies in the Extended Chandra Deep Field-South: The AGN Fraction and X-Ray Properties of Submillimeter Galaxies.

An extended Herschel drop-out source in the center of AS1063: a normal dusty galaxy at z = 6.1 or SZ substructures? (2013)
Journal Article
Boone, F., Clément, B., Richard, J., Schaerer, D., Lutz, D., Weiß, A., …Zamojski, M. (2013). An extended Herschel drop-out source in the center of AS1063: a normal dusty galaxy at z = 6.1 or SZ substructures?. Astronomy & Astrophysics, 559, Article L1. https://doi.org/10.1051/0004-6361/201322552

In the course of our 870 μm APEX/LABOCA follow-up of the Herschel Lensing Survey we have detected a source in AS1063 (RXC J2248.7-4431) that has no counterparts in any of the Herschel PACS/SPIRE bands, it is a Herschel “drop-out” with S870/S500 ≥ 0.5... Read More about An extended Herschel drop-out source in the center of AS1063: a normal dusty galaxy at z = 6.1 or SZ substructures?.

The SCUBA-2 Cosmology Legacy Survey: demographics of the 450-μm population (2013)
Journal Article
Roseboom, I., Dunlop, J., Cirasuolo, M., Geach, J., Smail, I., Halpern, M., …Zemcov, M. (2013). The SCUBA-2 Cosmology Legacy Survey: demographics of the 450-μm population. Monthly Notices of the Royal Astronomical Society, 436(1), 430-448. https://doi.org/10.1093/mnras/stt1577

We investigate the multiwavelength properties of a sample of 450-μm-selected sources from the SCUBA-2 Cosmology Legacy Survey. A total of 69 sources were identified above 4σ in deep SCUBA-2 450-μm observations overlapping the UDS and COSMOS fields an... Read More about The SCUBA-2 Cosmology Legacy Survey: demographics of the 450-μm population.

Herschel reveals the obscured star formation in HiZELS Hα emitters at z = 1.47 (2013)
Journal Article
Ibar, E., Sobral, D., Best, P., Ivison, R., Smail, I., Arumugam, V., …Zemcov, M. (2013). Herschel reveals the obscured star formation in HiZELS Hα emitters at z = 1.47. Monthly Notices of the Royal Astronomical Society, 434(4), 3218-3235. https://doi.org/10.1093/mnras/stt1258

We describe the far-infrared (far-IR; rest-frame 8–1000-μm) properties of a sample of 443 Hα-selected star-forming galaxies in the Cosmic Evolution Survey (COSMOS) and Ultra Deep Survey (UDS) fields detected by the High-redshift Emission Line Survey... Read More about Herschel reveals the obscured star formation in HiZELS Hα emitters at z = 1.47.

Using [C I] to probe the interstellar medium in z ∼ 2.5 sub-millimeter galaxies (2013)
Journal Article
Alaghband-Zadeh, S., Chapman, S., Swinbank, A., Smail, I., Danielson, A., Decarli, R., …van der Werf, P. (2013). Using [C I] to probe the interstellar medium in z ∼ 2.5 sub-millimeter galaxies. Monthly Notices of the Royal Astronomical Society, 435(2), 1493-1510. https://doi.org/10.1093/mnras/stt1390

We present new [C I](1–0) and 12CO(4–3) Plateau de Bure Interferometer observations of five sub-millimeter galaxies (SMGs) and combine these with all available [C I](1–0) literature detections in SMGs to probe the gas distribution within a sample of... Read More about Using [C I] to probe the interstellar medium in z ∼ 2.5 sub-millimeter galaxies.

X-ray emission around the z = 4.1 radio galaxy TN J1338-1942 and the potential role of far-infrared photons in AGN feedback (2013)
Journal Article
Smail, I., & Blundell, K. (2013). X-ray emission around the z = 4.1 radio galaxy TN J1338-1942 and the potential role of far-infrared photons in AGN feedback. Monthly Notices of the Royal Astronomical Society, 434(4), 3246-3251. https://doi.org/10.1093/mnras/stt1240

We report the discovery in an 80-ks observation of spatially extended X-ray emission around the high-redshift radio galaxy TN J1388−1942 (z = 4.11) with the Chandra X-ray Observatory. The X-ray emission extends over a ∼30-kpc diameter region and alth... Read More about X-ray emission around the z = 4.1 radio galaxy TN J1338-1942 and the potential role of far-infrared photons in AGN feedback.

On the evolution and environmental dependence of the star formation rate versus stellar mass relation since z ˜ 2 (2013)
Journal Article
Koyama, Y., Smail, I., Kurk, J., Geach, J. E., Sobral, D., Kodama, T., …Tadaki, K. (2013). On the evolution and environmental dependence of the star formation rate versus stellar mass relation since z ˜ 2. Monthly Notices of the Royal Astronomical Society, 434(1), 423-436. https://doi.org/10.1093/mnras/stt1035

This paper discusses the evolution of the correlation between galaxy star formation rates (SFRs) and stellar mass (M*) over the last ∼10 Gyr, particularly focusing on its environmental dependence. We first present the mid-infrared (MIR) properties of... Read More about On the evolution and environmental dependence of the star formation rate versus stellar mass relation since z ˜ 2.

e-MERLIN observations at 5 GHz of the GOODS-N region: pinpointing AGN cores in high-redshift galaxies (2013)
Journal Article
Guidetti, D., Bondi, M., Prandoni, I., Beswick, R., Muxlow, T., Wrigley, N., …McHardy, I. (2013). e-MERLIN observations at 5 GHz of the GOODS-N region: pinpointing AGN cores in high-redshift galaxies. Monthly Notices of the Royal Astronomical Society, 432(4), 2798-2807. https://doi.org/10.1093/mnras/stt633

We present 5 GHz e-Multi-Element Radio-Linked Interferometer Network (e-MERLIN) observations of the Great Observatories Origins Deep Surveys North (GOODS)-N region at sub-arcsec resolution (0.2–0.5 arcsec). These data form part of the early commissio... Read More about e-MERLIN observations at 5 GHz of the GOODS-N region: pinpointing AGN cores in high-redshift galaxies.

The SCUBA-2 cosmology legacy survey : blank-field number counts of 450-μm-selected galaxies and their contribution to the cosmic infrared background (2013)
Journal Article
Geach, J., Chapin, E., Coppin, K., Dunlop, J., Halpern, M., Smail, I., …Zemcov, M. (2013). The SCUBA-2 cosmology legacy survey : blank-field number counts of 450-μm-selected galaxies and their contribution to the cosmic infrared background. Monthly Notices of the Royal Astronomical Society, 432(1), 53-61. https://doi.org/10.1093/mnras/stt352

The first deep blank-field 450 μm map (1σ ≈ 1.3 mJy) from the Submillimetre Common-User Bolometer Array-2 SCUBA-2 Cosmology Legacy Survey (S2CLS), conducted with the James Clerk Maxwell Telescope (JCMT) is presented. Our map covers 140 arcmin2 of the... Read More about The SCUBA-2 cosmology legacy survey : blank-field number counts of 450-μm-selected galaxies and their contribution to the cosmic infrared background.

An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field South : high-resolution 870 μm source counts (2013)
Journal Article
Karim, A., Swinbank, A., Hodge, J., Smail, I., Walter, F., Biggs, A., …van der Werf, P. (2013). An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field South : high-resolution 870 μm source counts. Monthly Notices of the Royal Astronomical Society, 432(1), 2-9. https://doi.org/10.1093/mnras/stt196

We report the first counts of faint submillimetre galaxies (SMGs) in the 870-μm band derived from arcsecond-resolution observations with the Atacama Large Millimeter Array (ALMA). We have used ALMA to map a sample of 122 870-μm-selected submillimetre... Read More about An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field South : high-resolution 870 μm source counts.

An ALMA survey of submillimeter galaxies in the Extended Chandra Deep Field South : source catalog and multiplicity (2013)
Journal Article
Hodge, J., Karim, A., Smail, I., Swinbank, A., Walter, F., Biggs, A., …van der Werf, P. (2013). An ALMA survey of submillimeter galaxies in the Extended Chandra Deep Field South : source catalog and multiplicity. Astrophysical Journal, 768(1), Article 91. https://doi.org/10.1088/0004-637x/768/1/91

We present an Atacama Large Millimeter/submillimeter Array (ALMA) Cycle 0 survey of 126 submillimeter sources from the LABOCA ECDFS Submillimeter Survey (LESS). Our 870 μm survey with ALMA (ALESS) has produced maps ~3× deeper and with a beam area ~20... Read More about An ALMA survey of submillimeter galaxies in the Extended Chandra Deep Field South : source catalog and multiplicity.

SCUBA-2 : the 10 000 pixel bolometer camera on the James Clerk Maxwell telescope (2013)
Journal Article
Holland, W., Bintley, D., Chapin, E., Chrysostomou, A., Davis, G., Dempsey, J., …Thomas, H. (2013). SCUBA-2 : the 10 000 pixel bolometer camera on the James Clerk Maxwell telescope. Monthly Notices of the Royal Astronomical Society, 430(4), 2513-2533. https://doi.org/10.1093/mnras/sts612

Submillimetre Common-User Bolometer Array 2 (SCUBA-2) is an innovative 10 000 pixel bolometer camera operating at submillimetre wavelengths on the James Clerk Maxwell Telescope (JCMT). The camera has the capability to carry out wide-field surveys to... Read More about SCUBA-2 : the 10 000 pixel bolometer camera on the James Clerk Maxwell telescope.

Mapping the clumpy structures within submillimeter galaxies using laser-guide star adaptive optics spectroscopy (2013)
Journal Article
Menéndez-Delmestre, K., Blain, A., Swinbank, M., Smail, I., Ivison, R., Chapman, S., & Gonçalves, T. (2013). Mapping the clumpy structures within submillimeter galaxies using laser-guide star adaptive optics spectroscopy. Astrophysical Journal, 767(1), Article 151. https://doi.org/10.1088/0004-637x/767/2/151

We present the first integral-field spectroscopic observations of high-redshift submillimeter-selected galaxies (SMGs) using Laser-Guide Star Adaptive Optics. We target Hα emission of three SMGs at redshifts z ~ 1.4-2.4 with the OH-Suppressing Infrar... Read More about Mapping the clumpy structures within submillimeter galaxies using laser-guide star adaptive optics spectroscopy.

The merger rates and sizes of galaxies across the peak epoch of star formation from the HiZELS survey (2013)
Journal Article
Stott, J., Sobral, D., Smail, I., Bower, R., Best, P., & Geach, J. (2013). The merger rates and sizes of galaxies across the peak epoch of star formation from the HiZELS survey. Monthly Notices of the Royal Astronomical Society, 430(2), 1158-1170. https://doi.org/10.1093/mnras/sts684

We use the HiZELS narrow-band Hα survey in combination with CANDELS, UKIDSS and WIRDS near-infrared imaging, to investigate the morphologies, merger rates and sizes of a sample of Hα emitting galaxies in the redshift range z = 0.40-2.23, an epoch enc... Read More about The merger rates and sizes of galaxies across the peak epoch of star formation from the HiZELS survey.

Calibrating [O II] star formation rates at z < 1 from dual Hα-[O II] imaging from HiZELS (2013)
Journal Article
Hayashi, M., Sobral, D., Best, P., Smail, I., & Kodama, T. (2013). Calibrating [O II] star formation rates at z < 1 from dual Hα-[O II] imaging from HiZELS. Monthly Notices of the Royal Astronomical Society, 430(2), 1042-1050. https://doi.org/10.1093/mnras/sts676

We investigate the relationship between Hα and [O II](λ3727) emission in faint star-forming galaxies at z = 1.47 with dust uncorrected star formation rates (SFRs) down to 1.4 M⊙ yr-1, using data in two narrow bands from wide-field camera/United Kingd... Read More about Calibrating [O II] star formation rates at z < 1 from dual Hα-[O II] imaging from HiZELS.

Physical conditions of the gas in an ALMA [C II]-identified submillimetre galaxy at z = 4.44 (2013)
Journal Article
Huynh, M., Norris, R., Coppin, K., Emonts, B., Ivison, R., Seymour, N., …Weiss, A. (2013). Physical conditions of the gas in an ALMA [C II]-identified submillimetre galaxy at z = 4.44. Monthly Notices of the Royal Astronomical Society, 431(1), L88-L92. https://doi.org/10.1093/mnrasl/slt014

We present 12CO(2-1) observations of the submillimetre galaxy ALESS65.1 performed with the Australia Telescope Compact Array (ATCA) at 42.3 GHz. A previous Atacama Large Millimeter Array study of submillimetre galaxies (SMGs) in the Extended Chandra... Read More about Physical conditions of the gas in an ALMA [C II]-identified submillimetre galaxy at z = 4.44.

On the Effect of the Cosmic Microwave Background in High-redshift (Sub-)millimeter Observations (2013)
Journal Article
da Cunha, E., Groves, B., Walter, F., Decarli, R., Weiss, A., Bertoldi, F., …Smail, I. (2013). On the Effect of the Cosmic Microwave Background in High-redshift (Sub-)millimeter Observations. Astrophysical Journal, 766(1), Article 13. https://doi.org/10.1088/0004-637x/766/1/13

Modern (sub-)millimeter interferometers enable the measurement of the cool gas and dust emission of high-redshift galaxies (z > 5). However, at these redshifts the cosmic microwave background (CMB) temperature is higher, approaching, and even exceedi... Read More about On the Effect of the Cosmic Microwave Background in High-redshift (Sub-)millimeter Observations.

Concurrent supermassive black hole and galaxy growth : linking environment and nuclear activity in z = 2.23 H-alpha emitters (2013)
Journal Article
Lehmer, B., Lucy, A., Alexander, D., Best, P., Geach, J., Harrison, C., …Swinbank, A. (2013). Concurrent supermassive black hole and galaxy growth : linking environment and nuclear activity in z = 2.23 H-alpha emitters. Astrophysical Journal, 765(2), Article 87. https://doi.org/10.1088/0004-637x/765/2/87

We present results from a ≈100 ks Chandra observation of the 2QZ Cluster 1004+00 structure at z = 2.23 (hereafter 2QZ Clus). 2QZ Clus was originally identified as an overdensity of four optically-selected QSOs at z = 2.23 within a 15 × 15 arcmin2 reg... Read More about Concurrent supermassive black hole and galaxy growth : linking environment and nuclear activity in z = 2.23 H-alpha emitters.

Empirical Predictions for (Sub-)millimeter Line and Continuum Deep Fields (2013)
Journal Article
da Cunha, E., Walter, F., Decarli, R., Bertoldi, F., Carilli, C., Daddi, E., …Weiss, A. (2013). Empirical Predictions for (Sub-)millimeter Line and Continuum Deep Fields. Astrophysical Journal, 765(1), Article 9. https://doi.org/10.1088/0004-637x/765/1/9

Modern (sub-)millimeter/radio interferometers such as ALMA, JVLA, and the PdBI successor NOEMA will enable us to measure the dust and molecular gas emission from galaxies that have luminosities lower than the Milky Way, out to high redshifts and with... Read More about Empirical Predictions for (Sub-)millimeter Line and Continuum Deep Fields.

A survey of molecular gas in luminous sub-millimetre galaxies (2013)
Journal Article
Bothwell, M., Smail, I., Chapman, S., Genzel, R., Ivison, R., Tacconi, L., …Swinbank, A. (2013). A survey of molecular gas in luminous sub-millimetre galaxies. Monthly Notices of the Royal Astronomical Society, 429(4), 3047-3067. https://doi.org/10.1093/mnras/sts562

We present the results from a survey of 12CO emission in 40 luminous sub-millimetre galaxies (SMGs), with 850-μm fluxes of S850 μm = 4–20 mJy, conducted with the Plateau de Bure Interferometer. We detect 12CO emission in 32 SMGs at z ∼ 1.2–4.1, inclu... Read More about A survey of molecular gas in luminous sub-millimetre galaxies.

A large Hα survey at z = 2.23, 1.47, 0.84 and 0.40: the 11 Gyr evolution of star-forming galaxies from HiZELS (2013)
Journal Article
Sobral, D., Smail, I., Best, P., Geach, J., Matsuda, Y., Stott, J., …Kurk, J. (2013). A large Hα survey at z = 2.23, 1.47, 0.84 and 0.40: the 11 Gyr evolution of star-forming galaxies from HiZELS. Monthly Notices of the Royal Astronomical Society, 428(2), 1128-1146. https://doi.org/10.1093/mnras/sts096

This paper presents new deep and wide narrow-band surveys undertaken with United Kingdom Infrared Telescope (UKIRT), Subaru and the Very Large Telescope (VLT), a unique combined effort to select large, robust samples of Hα star-forming galaxies at z... Read More about A large Hα survey at z = 2.23, 1.47, 0.84 and 0.40: the 11 Gyr evolution of star-forming galaxies from HiZELS.

Massive starburst galaxies in a z = 2.16 proto-cluster unveiled by panoramic Hα mapping (2013)
Journal Article
Koyama, Y., Kodama, T., Tadaki, K., Hayashi, M., Tanaka, M., Smail, I., …Kurk, J. (2013). Massive starburst galaxies in a z = 2.16 proto-cluster unveiled by panoramic Hα mapping. Monthly Notices of the Royal Astronomical Society, 428(2), 1551-1564. https://doi.org/10.1093/mnras/sts133

We present a panoramic narrow-band study of Hα emitters in the field of the z = 2.16 proto-cluster around PKS 1138−262 using MOIRCS on the Subaru Telescope. We find 83 Hα emitters down to a star formation rate of SFR (Hα) ∼ 10 M⊙ yr−1 across a ∼ 7 ×... Read More about Massive starburst galaxies in a z = 2.16 proto-cluster unveiled by panoramic Hα mapping.

Herschel-ATLAS : a binary HyLIRG pinpointing a cluster of starbursting protoellipticals (2013)
Journal Article
Ivison, R., Swinbank, A., Smail, I., Harris, A., Bussmann, R., Cooray, A., …van der Wef, P. (2013). Herschel-ATLAS : a binary HyLIRG pinpointing a cluster of starbursting protoellipticals. Astrophysical Journal, 772(2), Article 137. https://doi.org/10.1088/0004-637x/772/2/137

Panchromatic observations of the best candidate hyperluminous infrared galaxies from the widest Herschel extragalactic imaging survey have led to the discovery of at least four intrinsically luminous z = 2.41 galaxies across an ≈100 kpc region—a clus... Read More about Herschel-ATLAS : a binary HyLIRG pinpointing a cluster of starbursting protoellipticals.

The VISTA Deep Extragalactic Observations (VIDEO) survey (2013)
Journal Article
Jarvis, M., Bonfield, D., Bruce, V., Geach, J., McAlpine, K., McLure, R., …Zwart, J. (2013). The VISTA Deep Extragalactic Observations (VIDEO) survey. Monthly Notices of the Royal Astronomical Society, 428(2), 1281-1295. https://doi.org/10.1093/mnras/sts118

In this paper, we describe the first data release of the Visible and Infrared Survey Telescope for Astronomy (VISTA) Deep Extragalactic Observations (VIDEO) survey. VIDEO is a ∼12 deg2 survey in the near-infrared Z, Y, J, H and Ks bands, specifically... Read More about The VISTA Deep Extragalactic Observations (VIDEO) survey.

An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field-South: detection of [C II] at z = 4.4 (2012)
Journal Article
Swinbank, A., Karim, A., Smail, I., Hodge, J., Walter, F., Bertoldi, F., …van der Werf, P. (2012). An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field-South: detection of [C II] at z = 4.4. Monthly Notices of the Royal Astronomical Society, 427(2), 1066-1074. https://doi.org/10.1111/j.1365-2966.2012.22048.x

We present Atacama Large Millimeter Array (ALMA) 870-μm (345-GHz) observations of two submillimetre galaxies (SMGs) drawn from an ALMA study of the 126 submillimetre sources from the LABOCA Extended Chandra Deep Field-South Survey (LESS). The ALMA da... Read More about An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field-South: detection of [C II] at z = 4.4.

Inverse Compton X-ray halos around high-z radio galaxies : a feedback mechanism powered by far-infrared starbursts or the cosmic microwave background? (2012)
Journal Article
Smail, I., Blundell, K., Lehmer, B., & Alexander, D. (2012). Inverse Compton X-ray halos around high-z radio galaxies : a feedback mechanism powered by far-infrared starbursts or the cosmic microwave background?. Astrophysical Journal, 760(2), Article 132. https://doi.org/10.1088/0004-637x/760/2/132

We report the detection of extended X-ray emission around two powerful radio galaxies at z ~ 3.6 (4C 03.24 and 4C 19.71) and use these to investigate the origin of extended, inverse Compton (IC) powered X-ray halos at high redshifts. The halos have X... Read More about Inverse Compton X-ray halos around high-z radio galaxies : a feedback mechanism powered by far-infrared starbursts or the cosmic microwave background?.

Herschel-PACS observations of [O I]63 μm towards submillimetre galaxies at z ˜ 1 (2012)
Journal Article
Coppin, K., Danielson, A., Geach, J., Hodge, J., Swinbank, A., Wardlow, J., …van der Werf, P. (2012). Herschel-PACS observations of [O I]63 μm towards submillimetre galaxies at z ˜ 1. Monthly Notices of the Royal Astronomical Society, 427(1), 520-532. https://doi.org/10.1111/j.1365-2966.2012.21977.x

We present Herschel-PACS spectroscopy of the [O I]63 μm far-infrared cooling line from a sample of six unlensed and spectroscopically confirmed 870 μm selected submillimetre (submm) galaxies (SMGs) at 1.1 < z < 1.6 from the LABOCA Extended Chandra De... Read More about Herschel-PACS observations of [O I]63 μm towards submillimetre galaxies at z ˜ 1.

The evolutionary connection between QSOs and SMGs: molecular gas in far-infrared luminous QSOs at z \tilde 2.5 (2012)
Journal Article
Simpson, J., Smail, I., Swinbank, A., Alexander, D., Auld, R., Baes, M., …van der Werf, P. (2012). The evolutionary connection between QSOs and SMGs: molecular gas in far-infrared luminous QSOs at z \tilde 2.5. Monthly Notices of the Royal Astronomical Society, 426(4), 3201-3210. https://doi.org/10.1111/j.1365-2966.2012.21941.x

We present Institut de Radioastronomie Millimétrique Plateau de Bure Interferometer observations of the 12CO (3–2) emission from two far-infrared luminous QSOs at z ∼ 2.5 selected from the Herschel-Astrophysical Tetrahertz Large Area Survey. These fa... Read More about The evolutionary connection between QSOs and SMGs: molecular gas in far-infrared luminous QSOs at z \tilde 2.5.

Hubble Space Telescope Hα imaging of star-forming galaxies at z ≃ 1–1.5 : evolution in the size and luminosity of giant H ii regions (2012)
Journal Article
Livermore, R., Jones, T., Richard, J., Bower, R., Ellis, R., Swinbank, A., …Crain, R. (2012). Hubble Space Telescope Hα imaging of star-forming galaxies at z ≃ 1–1.5 : evolution in the size and luminosity of giant H ii regions. Monthly Notices of the Royal Astronomical Society, 427(1), 688-702. https://doi.org/10.1111/j.1365-2966.2012.21900.x

We present Hubble Space Telescope/Wide Field Camera 3 narrow-band imaging of the Hα emission in a sample of eight gravitationally lensed galaxies at z = 1–1.5. The magnification caused by the foreground clusters enables us to obtain a median source p... Read More about Hubble Space Telescope Hα imaging of star-forming galaxies at z ≃ 1–1.5 : evolution in the size and luminosity of giant H ii regions.

AzTEC half square degree survey of the SHADES fields - II : identifications, redshifts and evidence for large-scale structure (2012)
Journal Article
Michaelowski, M., Dunlop, J., Ivison, R., Cirasuolo, M., Caputi, K., Aretxaga, I., …Yun, M. (2012). AzTEC half square degree survey of the SHADES fields - II : identifications, redshifts and evidence for large-scale structure. Monthly Notices of the Royal Astronomical Society, 426(3), 1845-1866. https://doi.org/10.1111/j.1365-2966.2012.21828.x

The Astronomical Thermal Emission Camera (AzTEC) 1.1 mm survey of the two SCUBA HAlf Degree Extragalactic Survey (SHADES) fields is the largest (0.7 deg2) blank-field millimetre-wavelength (mm-wavelength) survey undertaken to date at a resolution of... Read More about AzTEC half square degree survey of the SHADES fields - II : identifications, redshifts and evidence for large-scale structure.

The properties of the star-forming interstellar medium at z = 0.84-2.23 from HiZELS : mapping the internal dynamics and metallicity gradients in high-redshift disc galaxies (2012)
Journal Article
Swinbank, A., Sobral, D., Smail, I., Geach, J., Best, P., McCarthy, I., …Theuns, T. (2012). The properties of the star-forming interstellar medium at z = 0.84-2.23 from HiZELS : mapping the internal dynamics and metallicity gradients in high-redshift disc galaxies. Monthly Notices of the Royal Astronomical Society, 426(2), 935-950. https://doi.org/10.1111/j.1365-2966.2012.21774.x

We present adaptive optics assisted, spatially resolved spectroscopy of a sample of nine Hα-selected galaxies at z = 0.84-2.23 drawn from the HiZELS narrow-band survey. These galaxies have star formation rates of 1-27 M⊙ yr-1 and are therefore repres... Read More about The properties of the star-forming interstellar medium at z = 0.84-2.23 from HiZELS : mapping the internal dynamics and metallicity gradients in high-redshift disc galaxies.

The clustering of Hα emitters at z = 2.23 from HiZELS (2012)
Journal Article
Geach, J., Sobral, D., Hickox, R., Wake, D., Smail, I., Best, P., …Stott, J. (2012). The clustering of Hα emitters at z = 2.23 from HiZELS. Monthly Notices of the Royal Astronomical Society, 426(1), 679-689. https://doi.org/10.1111/j.1365-2966.2012.21725.x

We present a clustering analysis of 370 high-confidence Hα emitters (HAEs) at z = 2.23. The HAEs are detected in the Hi-Z Emission Line Survey (HiZELS), a large-area blank field 2.121 μm narrow-band survey using the United Kingdom Infrared Telescope... Read More about The clustering of Hα emitters at z = 2.23 from HiZELS.

Gas-rich mergers and feedback are ubiquitous amongst starbursting radio galaxies, as revealed by the VLA, IRAM PdBI and Herschel (2012)
Journal Article
Ivison, R., Smail, I., Amblard, A., Arumugam, V., De Breuck, C., Emonts, B., …Wylezalek, D. (2012). Gas-rich mergers and feedback are ubiquitous amongst starbursting radio galaxies, as revealed by the VLA, IRAM PdBI and Herschel. Monthly Notices of the Royal Astronomical Society, 425(2), 1320-1331. https://doi.org/10.1111/j.1365-2966.2012.21544.x

We report new, sensitive observations of two z ˜ 3-3.5 far-infrared-luminous radio galaxies, 6C 1909+72 and B3 J2330+3927, in the 12CO J = 1-0 transition with the Karl Jansky Very Large Array and at 100-500 m using Herschel, alongside new and archiva... Read More about Gas-rich mergers and feedback are ubiquitous amongst starbursting radio galaxies, as revealed by the VLA, IRAM PdBI and Herschel.

VLA imaging of 12CO J = 1-0 and free-free emission in lensed submillimetre galaxies (2012)
Journal Article
Thomson, A., Ivison, R., Smail, I., Swinbank, A., Weiss, A., Kneib, J., …van Moorsel, G. (2012). VLA imaging of 12CO J = 1-0 and free-free emission in lensed submillimetre galaxies. Monthly Notices of the Royal Astronomical Society, 425(3), 2203-2211. https://doi.org/10.1111/j.1365-2966.2012.21584.x

We present a study using the Karl G. Jansky Very Large Array (VLA) of 12CO J = 1-0 emission in three strongly lensed submillimetre-selected galaxies (SMM J16359, SMM J14009 and SMM J02399) at z = 2.5-2.9. These galaxies span LIR = 1011-1013 L⊙, offer... Read More about VLA imaging of 12CO J = 1-0 and free-free emission in lensed submillimetre galaxies.

Integral field spectroscopy of 2.0 < z < 2.7 submillimetre galaxies : gas morphologies and kinematics (2012)
Journal Article
Alaghband-Zadeh, S., Chapman, S., Swinbank, A., Smail, I., Harrison, C., Alexander, D., …Umehata, H. (2012). Integral field spectroscopy of 2.0 < z < 2.7 submillimetre galaxies : gas morphologies and kinematics. Monthly Notices of the Royal Astronomical Society, 424(3), 2232-2248. https://doi.org/10.1111/j.1365-2966.2012.21386.x

We present 2D, integral field spectroscopy covering the rest-frame wavelengths of strong optical emission lines in nine submillimetre luminous galaxies (SMGs) at 2.0 < z < 2.7. The Gemini-North/Near-Infrared Integral Field Spectrograph (NIFS) and Ver... Read More about Integral field spectroscopy of 2.0 < z < 2.7 submillimetre galaxies : gas morphologies and kinematics.

Strong lensing by a node of the cosmic web. The core of MACS J0717.5+3745 at z = 0.55 (2012)
Journal Article
Limousin, M., Ebeling, H., Richard, J., Swinbank, A., Smith, G., Jauzac, M., …Kneib, J. (2012). Strong lensing by a node of the cosmic web. The core of MACS J0717.5+3745 at z = 0.55. Astronomy & Astrophysics, 544, Article A71. https://doi.org/10.1051/0004-6361/201117921

We present results of a strong-lensing analysis of MACS J0717.5+3745 (hereafter MACS J0717), an extremely X-ray luminous galaxy cluster at z = 0.55. Observations at different wavelengths reveal a complex and dynamically very active cluster, whose cor... Read More about Strong lensing by a node of the cosmic web. The core of MACS J0717.5+3745 at z = 0.55.

The LABOCA survey of the Extended Chandra Deep Field-South: clustering of submillimetre galaxies (2012)
Journal Article
Hickox, R., Wardlow, J., Smail, I., Myers, A., Alexander, D., Swinbank, A., …Weiss, A. (2012). The LABOCA survey of the Extended Chandra Deep Field-South: clustering of submillimetre galaxies. Monthly Notices of the Royal Astronomical Society, 421(1), 284-295. https://doi.org/10.1111/j.1365-2966.2011.20303.x

We present a measurement of the spatial clustering of submillimetre galaxies (SMGs) at z= 1–3. Using data from the 870 μm Large APEX Bolometer Camera (LABOCA) submillimetre survey of the Extended Chandra Deep Field-South, we employ a novel technique... Read More about The LABOCA survey of the Extended Chandra Deep Field-South: clustering of submillimetre galaxies.

A Herschel view of the far-infrared properties of submillimetre galaxies (2012)
Journal Article
Magnelli, B., Lutz, D., Santini, P., Saintonge, A., Berta, S., Albrecht, M., …Wuyts, S. (2012). A Herschel view of the far-infrared properties of submillimetre galaxies. Astronomy & Astrophysics, 539, Article A155. https://doi.org/10.1051/0004-6361/201118312

We study a sample of 61submillimetre galaxies (SMGs) selected from ground-based surveys, with known spectroscopic redshifts and observed with the Herschel Space Observatory as part of the PACS Evolutionary Probe (PEP) and the Herschel Multi-tiered Ex... Read More about A Herschel view of the far-infrared properties of submillimetre galaxies.

Star formation at z=1.47 from HiZELS : an Hα+ [O II] double-blind study (2012)
Journal Article
Sobral, D., Best, P., Matsuda, Y., Smail, I., Geach, J., & Cirasuolo, M. (2012). Star formation at z=1.47 from HiZELS : an Hα+ [O II] double-blind study. Monthly Notices of the Royal Astronomical Society, 420(3), 1926-1945. https://doi.org/10.1111/j.1365-2966.2011.19977.x

This paper presents the results from the first wide and deep dual narrow-band survey to select Hα and [O II] line emitters at z= 1.47 ± 0.02, exploiting synergies between the United Kingdom Infrared Telescope and the Subaru telescope by using matched... Read More about Star formation at z=1.47 from HiZELS : an Hα+ [O II] double-blind study.

A bright z = 5.2 lensed submillimeter galaxy in the field of Abell 773 : HLSJ091828.6+514223 (2012)
Journal Article
Combes, F., Rex, M., Rawle, T., Egami, E., Boone, F., Smail, I., …van der Werf, P. (2012). A bright z = 5.2 lensed submillimeter galaxy in the field of Abell 773 : HLSJ091828.6+514223. Astronomy & Astrophysics, 538, Article L4. https://doi.org/10.1051/0004-6361/201118750

During our Herschel Lensing Survey (HLS) of massive galaxy clusters, we have discovered an exceptionally bright source behind the z = 0.22 cluster Abell 773, which appears to be a strongly lensed submillimeter galaxy (SMG) at z = 5.2429. This source... Read More about A bright z = 5.2 lensed submillimeter galaxy in the field of Abell 773 : HLSJ091828.6+514223.

The Interstellar Medium in Distant Star-forming Galaxies: Turbulent Pressure, Fragmentation, and Cloud Scaling Relations in a Dense Gas Disk at z = 2.3 (2011)
Journal Article
Swinbank, A., Papadopoulos, P., Cox, P., Krips, M., Ivison, R., Smail, I., …Ebeling, H. (2011). The Interstellar Medium in Distant Star-forming Galaxies: Turbulent Pressure, Fragmentation, and Cloud Scaling Relations in a Dense Gas Disk at z = 2.3. Astrophysical Journal, 742(1), Article 11. https://doi.org/10.1088/0004-637x/742/1/11

The stellar mass content of submillimeter-selected galaxies (2011)
Journal Article
Hainline, L., Blain, A., Smail, I., Alexander, D., Armus, L., Chapman, S., & Ivison, R. (2011). The stellar mass content of submillimeter-selected galaxies. Astrophysical Journal, 740(2), Article 96. https://doi.org/10.1088/0004-637x/740/2/96

We present a new study of stellar mass in a sample of ~70 submillimeter-selected galaxies (SMGs) with accurate spectroscopic redshifts. We fit combinations of stellar population synthesis models and power laws to the galaxies' observed-frame optical... Read More about The stellar mass content of submillimeter-selected galaxies.

Far-infrared constraints on the contamination by dust-obscured galaxies of high-z dropout searches (2011)
Journal Article
Boone, F., Schaerer, D., Pelló, R., Lutz, D., Weiss, A., Egami, E., …Menten, K. (2011). Far-infrared constraints on the contamination by dust-obscured galaxies of high-z dropout searches. Astronomy & Astrophysics, 534, Article A124. https://doi.org/10.1051/0004-6361/201117338

The spectral energy distributions (SED) of dusty galaxies at intermediate redshift may look similar to very high-redshift galaxies in the optical/near infrared (NIR) domain. This can lead to the contamination of high-redshift galaxy searches based on... Read More about Far-infrared constraints on the contamination by dust-obscured galaxies of high-z dropout searches.

Herschel-Astrophysical Terahertz Large Area Survey: detection of a far-infrared population around galaxy clusters (2011)
Journal Article
Coppin, K., Geach, J., Smail, I., Dunne, L., Edge, A., Ivison, R., …van der Werf, P. (2011). Herschel-Astrophysical Terahertz Large Area Survey: detection of a far-infrared population around galaxy clusters. Monthly Notices of the Royal Astronomical Society, 416(1), 680-688. https://doi.org/10.1111/j.1365-2966.2011.19084.x

We report the detection of a significant excess in the surface density of far-infrared sources from the Herschel-Astrophysical Terahertz Large Area Survey within ∼1 Mpc of the centres of 66 optically selected clusters of galaxies in the Sloan Digital... Read More about Herschel-Astrophysical Terahertz Large Area Survey: detection of a far-infrared population around galaxy clusters.

Physical conditions of the interstellar medium of high-redshift, strongly lensed submillimetre galaxies from the Herschel-ATLAS (2011)
Journal Article
Valtchanov, I., Virdee, J., Ivison, R., Swinyard, B., van der Werf, P., Rigopoulou, D., …Vieira, J. (2011). Physical conditions of the interstellar medium of high-redshift, strongly lensed submillimetre galaxies from the Herschel-ATLAS. Monthly Notices of the Royal Astronomical Society, 415, 3473-3484. https://doi.org/10.1111/j.1365-2966.2011.18959.x

The LABOCA survey of the Extended Chandra Deep Field-South : a photometric redshift survey of submillimetre galaxies (2011)
Journal Article
Wardlow, J., Smail, I., Coppin, K., Alexander, D., Brandt, W., Danielson, A., …van der Werf, P. (2011). The LABOCA survey of the Extended Chandra Deep Field-South : a photometric redshift survey of submillimetre galaxies. Monthly Notices of the Royal Astronomical Society, 415(2), 1479-1508. https://doi.org/10.1111/j.1365-2966.2011.18795.x

We derive photometric redshifts from 17-band optical to mid-infrared photometry of 78 robust radio, 24-μm and Spitzer IRAC counterparts to 72 of the 126 submillimetre galaxies (SMGs) selected at 870 μm by LABOCA observations in the Extended Chandra D... Read More about The LABOCA survey of the Extended Chandra Deep Field-South : a photometric redshift survey of submillimetre galaxies.

Observation of H2O in a strongly lensed Herschel-ATLAS source at z=2.3 (2011)
Journal Article
Omont, A., Neri, R., Cox, P., Lupu, R., Guélin, M., van der Werf, P., …Zmuidzinas, J. (2011). Observation of H2O in a strongly lensed Herschel-ATLAS source at z=2.3. Astronomy & Astrophysics, 530, Article L3. https://doi.org/10.1051/0004-6361/201116921

The Herschel survey, H-ATLAS, with its large areal coverage, has recently discovered a number of bright, strongly lensed high-z submillimeter galaxies. The strong magnification makes it possible to study molecular species other than CO, which are oth... Read More about Observation of H2O in a strongly lensed Herschel-ATLAS source at z=2.3.

The properties of the interstellar medium within a star-forming galaxy at z= 2.3 (2011)
Journal Article
Danielson, A., Swinbank, A., Smail, I., Cox, P., Edge, A., Weiss, A., …Flaquer, B. (2011). The properties of the interstellar medium within a star-forming galaxy at z= 2.3. Monthly Notices of the Royal Astronomical Society, 410(3), 1687-1702. https://doi.org/10.1111/j.1365-2966.2010.17549.x

We present an analysis of the molecular and atomic gas emission in the rest-frame far-infrared and submillimetre from the lensed z= 2.3 submillimetre galaxy SMM J2135−0102. We obtain very high signal-to-noise ratio detections of 11 transitions from t... Read More about The properties of the interstellar medium within a star-forming galaxy at z= 2.3.

The evolution of galaxy clustering since z = 3 using the UKIDSS Ultra Deep Survey: the divergence of passive and star-forming galaxies (2010)
Journal Article
Hartley, W., Almaini, O., Cirasuolo, M., Foucaud, S., Simpson, C., Conselice, C., …Bradshaw, E. (2010). The evolution of galaxy clustering since z = 3 using the UKIDSS Ultra Deep Survey: the divergence of passive and star-forming galaxies. Monthly Notices of the Royal Astronomical Society, 407, 1212-1222. https://doi.org/10.1111/j.1365-2966.2010.16972.x

Herschel and SCUBA-2 imaging and spectroscopy of a bright, lensed submillimetre galaxy at z = 2.3 (2010)
Journal Article
Ivison, R., Swinbank, A., Swinyard, B., Smail, I., Pearson, C., Rigopoulou, D., …Wright, G. (2010). Herschel and SCUBA-2 imaging and spectroscopy of a bright, lensed submillimetre galaxy at z = 2.3. Astronomy & Astrophysics, 518, Article L35. https://doi.org/10.1051/0004-6361/201014548

We present a detailed analysis of the far-infrared (-IR) properties of the bright, lensed, z = 2.3, submillimetre-selected galaxy (SMG), SMM J2135-0102 (hereafter SMM J2135), using new observations with Herschel, SCUBA-2 and the Very Large Array (VLA... Read More about Herschel and SCUBA-2 imaging and spectroscopy of a bright, lensed submillimetre galaxy at z = 2.3.

The far-infrared/submillimeter properties of galaxies located behind the Bullet cluster (2010)
Journal Article
Rex, M., Rawle, T., Egami, E., Pérez-Gonzá&lez, P., Zemcov, M., Aretxaga, I., …Yun, M. (2010). The far-infrared/submillimeter properties of galaxies located behind the Bullet cluster. Astronomy & Astrophysics, 518, Article L13. https://doi.org/10.1051/0004-6361/201014693

The Herschel Lensing Survey (HLS) takes advantage of gravitational lensing by massive galaxy clusters to sample a population of high-redshift galaxies which are too faint to be detected above the confusion limit of current far-infrared/submillimeter... Read More about The far-infrared/submillimeter properties of galaxies located behind the Bullet cluster.

Deep Herschel view of obscured star formation in the Bullet cluster (2010)
Journal Article
Rawle, T., Chung, S., Fadda, D., Rex, M., Egami, E., Pérez-Gonzá&lez, P., …Werner, M. (2010). Deep Herschel view of obscured star formation in the Bullet cluster. Astronomy & Astrophysics, 518, Article L14. https://doi.org/10.1051/0004-6361/201014681

We use deep, five band (100–500 μm) data from the Herschel Lensing Survey (HLS) to fully constrain the obscured star formation rate, SFRFIR, of galaxies in the Bullet cluster (z = 0.296), and a smaller background system (z = 0.35) in the same field.... Read More about Deep Herschel view of obscured star formation in the Bullet cluster.

The Herschel Lensing Survey (HLS) : Overview (2010)
Journal Article
Egami, E., Rex, M., Rawle, T., Pérez-Gonzá&lez, P., Richard, J., Kneib, J., …Werner, M. (2010). The Herschel Lensing Survey (HLS) : Overview. Astronomy & Astrophysics, 518, Article L12. https://doi.org/10.1051/0004-6361/201014696

The Herschel Lensing Survey (HLS) will conduct deep PACS and SPIRE imaging of ~40 massive clusters of galaxies. The strong gravitational lensing power of these clusters will enable us to penetrate through the confusion noise, which sets the ultimate... Read More about The Herschel Lensing Survey (HLS) : Overview.

Mid-infrared spectroscopy of candidate active galactic nuclei-dominated submillimeter galaxies (2010)
Journal Article
Coppin, K., Pope, A., Menéndez-Delmestre, K., Alexander, D., Dunlop, J., Egami, E., …Yun, M. (2010). Mid-infrared spectroscopy of candidate active galactic nuclei-dominated submillimeter galaxies. Astrophysical Journal, 713(1), 503-519. https://doi.org/10.1088/0004-637x/713/1/503

Spitzer spectroscopy has revealed that sime80% of submm galaxies (SMGs) are starburst (SB)-dominated in the mid-infrared. Here we focus on the remaining sime20% that show signs of harboring powerful active galactic nuclei (AGNs). We have obtained Spi... Read More about Mid-infrared spectroscopy of candidate active galactic nuclei-dominated submillimeter galaxies.

The Herschel ATLAS (2010)
Journal Article
Eales, S., Dunne, L., Clements, D., Cooray, A., de Zotti, G., Dye, S., …White, G. (2010). The Herschel ATLAS. Publications of the Astronomical Society of the Pacific, 122(891), 499-515. https://doi.org/10.1086/653086

The Herschel ATLAS is the largest open-time key project that will be carried out on the Herschel Space Observatory. It will survey 570 deg2 of the extragalactic sky, 4 times larger than all the other Herschel extragalactic surveys combined, in five f... Read More about The Herschel ATLAS.

The LABOCA survey of the extended Chandra Deep Field South : two modes of star formation in active galactic nucleus hosts? (2010)
Journal Article
Lutz, D., Mainieri, V., Rafferty, D., Shao, L., Hasinger, G., Weiß, A., …Xue, Y. (2010). The LABOCA survey of the extended Chandra Deep Field South : two modes of star formation in active galactic nucleus hosts?. Astrophysical Journal, 712(2), 1287-1301. https://doi.org/10.1088/0004-637x/712/2/1287

We study the co-existence of star formation and active galactic nucleus (AGN) activity in Chandra X-ray-selected AGN by analyzing stacked 870 μm submillimeter emission from a deep and wide map of the Extended Chandra Deep Field South (ECDFS), obtaine... Read More about The LABOCA survey of the extended Chandra Deep Field South : two modes of star formation in active galactic nucleus hosts?.

Obscured star formation at z = 0.84 with HiZELS: the relationship between star formation rate and H$\alpha$ or ultraviolet dust extinction (2010)
Journal Article
Garn, T., Sobral, D., Best, P., Geach, J., Smail, I., Cirasuolo, M., …Farrah, D. (2010). Obscured star formation at z = 0.84 with HiZELS: the relationship between star formation rate and H$\alpha$ or ultraviolet dust extinction. Monthly Notices of the Royal Astronomical Society, 402, 2017-2030. https://doi.org/10.1111/j.1365-2966.2009.16042.x

An AzTEC 1.1-mm survey for ULIRGs in the field of the Galaxy Cluster MS0451.6-0305 (2010)
Journal Article
Wardlow, J., Smail, I., Wilson, G., Yun, M., Coppin, K., Cybulski, R., …Scott, K. (2010). An AzTEC 1.1-mm survey for ULIRGs in the field of the Galaxy Cluster MS0451.6-0305. Monthly Notices of the Royal Astronomical Society, 401(4), 2299-2317. https://doi.org/10.1111/j.1365-2966.2009.15847.x

We have undertaken a deep (σ∼ 1.1 mJy) 1.1-mm survey of the z= 0.54 cluster MS 0451.6−0305 using the AzTEC camera on the James Clerk Maxwell Telescope. We detect 36 sources with signal-to-noise ratio (S/N) ≥ 3.5 in the central 0.10 deg2 and present t... Read More about An AzTEC 1.1-mm survey for ULIRGs in the field of the Galaxy Cluster MS0451.6-0305.

AzTEC half square degree survey of the SHADES fields - I. Maps, catalogues and source counts (2010)
Journal Article
Austermann, J., Dunlop, J., Perera, T., Scott, K., Wilson, G., Aretxaga, I., …Yun, M. (2010). AzTEC half square degree survey of the SHADES fields - I. Maps, catalogues and source counts. Monthly Notices of the Royal Astronomical Society, 401(1), 160-176. https://doi.org/10.1111/j.1365-2966.2009.15620.x

We present the first results from the largest deep extragalactic mm-wavelength survey undertaken to date. These results are derived from maps covering over 0.7 deg2, made at λ= 1.1 mm, using the AzTEC continuum camera mounted on the James Clerk Maxwe... Read More about AzTEC half square degree survey of the SHADES fields - I. Maps, catalogues and source counts.

The Large Apex Bolometer camera survey of the Extended Chandra Deep Field South (2009)
Journal Article
Weiß, A., Kovács, A., Coppin, K., Greve, T., Walter, F., Smail, I., …van der Werf, P. (2009). The Large Apex Bolometer camera survey of the Extended Chandra Deep Field South. Astrophysical Journal, 707(2), 1201-1216. https://doi.org/10.1088/0004-637x/707/2/1201

We present a sensitive 870 μm survey of the Extended Chandra Deep Field South (ECDFS) combining 310 hr of observing time with the Large Apex BOlometer Camera (LABOCA) on the APEX telescope. The LABOCA ECDFS Submillimetre Survey (LESS) covers the full... Read More about The Large Apex Bolometer camera survey of the Extended Chandra Deep Field South.

Ly$\alpha$ blobs like company: the discovery of a candidate 100kpc Ly$\alpha$ blob near to a radio galaxy with a giant Ly$\alpha$ halo B3J2330+3927 at z = 3.1 (2009)
Journal Article
Matsuda, Y., Nakamura, Y., Morimoto, N., Smail, I., De Breuck, C., Ohta, K., …Hibon, P. (2009). Ly$\alpha$ blobs like company: the discovery of a candidate 100kpc Ly$\alpha$ blob near to a radio galaxy with a giant Ly$\alpha$ halo B3J2330+3927 at z = 3.1. Monthly Notices of the Royal Astronomical Society: Letters, 400, L66-L70. https://doi.org/10.1111/j.1745-3933.2009.00764.x

The Chandra Deep protocluster survey : Lyα blobs are powered by heating, not cooling (2009)
Journal Article
Geach, J., Alexander, D., Lehmer, B., Smail, I., Matsuda, Y., Chapman, S., …Basu-Zych, A. (2009). The Chandra Deep protocluster survey : Lyα blobs are powered by heating, not cooling. Astrophysical Journal, 700(1), 1-9. https://doi.org/10.1088/0004-637x/700/1/1

We present the results of a 400 ks Chandra survey of 29 extended Lyα emitting nebulae (Lyα Blobs, LABs) in the z = 3.09 protocluster in the SS A22 field. We detect luminous X-ray counterparts in five LABs, implying a large fraction of active galactic... Read More about The Chandra Deep protocluster survey : Lyα blobs are powered by heating, not cooling.

Mid-infrared spectroscopy of submillimeter galaxies : extended star formation in massive high-redshift galaxies (2009)
Journal Article
Menéndez-Delmestre, K., Blain, A., Smail, I., Alexander, D., Chapman, S., Armus, L., …Teplitz, H. (2009). Mid-infrared spectroscopy of submillimeter galaxies : extended star formation in massive high-redshift galaxies. Astrophysical Journal, 699(1), 667-685. https://doi.org/10.1088/0004-637x/699/1/667

We used the Spitzer Infrared Spectrograph (IRS) to study the mid-IR properties and investigate the energetics of 24 Submillimeter Galaxies (SMGs). This is the largest sample of SMGs observed with Spitzer IRS and covers the full extent of properties o... Read More about Mid-infrared spectroscopy of submillimeter galaxies : extended star formation in massive high-redshift galaxies.

A mid-infrared imaging survey of submillimeter-selected galaxies with the Spitzer space telescope (2009)
Journal Article
Hainline, L., Blain, A., Smail, I., Frayer, D., Chapman, S., Ivison, R., & Alexander, D. (2009). A mid-infrared imaging survey of submillimeter-selected galaxies with the Spitzer space telescope. Astrophysical Journal, 699(2), 1610-1632. https://doi.org/10.1088/0004-637x/699/2/1610

We present Spitzer-IRAC and MIPS mid-IR observations of a sample of 73 radio-detected submillimeter-selected galaxies (SMGs) with spectroscopic redshifts, the largest such sample published to date. From our data, we find that IRAC colors of SMGs are... Read More about A mid-infrared imaging survey of submillimeter-selected galaxies with the Spitzer space telescope.

Detection of Far-Infrared and Polycyclic Aromatic Hydrocarbon Emission from the Cosmic Eye: Probing the Dust and Star Formation of Lyman Break Galaxies (2009)
Journal Article
Siana, B., Smail, I., Swinbank, A., Richard, J., Teplitz, H., Coppin, K., …Edge, A. (2009). Detection of Far-Infrared and Polycyclic Aromatic Hydrocarbon Emission from the Cosmic Eye: Probing the Dust and Star Formation of Lyman Break Galaxies. Astrophysical Journal, 698(2), 1273-1281. https://doi.org/10.1088/0004-637x/698/2/1273

We report the results of a Spitzer infrared (IR) study of the Cosmic Eye, a strongly lensed, L*UV Lyman break galaxy (LBG) at z = 3.074. We obtained Spitzer mid-IR spectroscopy as well as MIPS 24 and 70 μm photometry. The Eye is detected with high si... Read More about Detection of Far-Infrared and Polycyclic Aromatic Hydrocarbon Emission from the Cosmic Eye: Probing the Dust and Star Formation of Lyman Break Galaxies.

SPACE: the spectroscopic all-sky cosmic explorer (2009)
Journal Article
Cimatti, A., Robberto, M., Baugh, C., Beckwith, S., Content, R., Daddi, E., …Zerbi, F. (2009). SPACE: the spectroscopic all-sky cosmic explorer. Experimental Astronomy, 23(1), 39-66. https://doi.org/10.1007/s10686-008-9096-7

We describe the scientific motivations, the mission concept and the instrumentation of SPACE, a class-M mission proposed for concept study at the first call of the ESA Cosmic-Vision 2015–2025 planning cycle. SPACE aims to produce the largest three-di... Read More about SPACE: the spectroscopic all-sky cosmic explorer.

The Chandra Deep protocluster survey : evidence for an enhancement of AGN activity in the SSA22 protocluster at z = 3.09 (2009)
Journal Article
Lehmer, B., Alexander, D., Geach, J., Smail, I., Basu-Zych, A., Bauer, F., …Yamada, T. (2009). The Chandra Deep protocluster survey : evidence for an enhancement of AGN activity in the SSA22 protocluster at z = 3.09. Astrophysical Journal, 691(1), 687-695. https://doi.org/10.1088/0004-637x/691/1/687

We present results from a new ultra-deep ≈400 ks Chandra observation of the SSA22 protocluster at z = 3.09. We have studied the X-ray properties of 234 z ~ 3 Lyman Break Galaxies (LBGs; protocluster and field) and 158 z = 3.09 Lyα Emitters (LAEs) in... Read More about The Chandra Deep protocluster survey : evidence for an enhancement of AGN activity in the SSA22 protocluster at z = 3.09.

The properties of submm galaxies in hierarchical models (2008)
Journal Article
Swinbank, A., Lacey, C., Smail, I., Baugh, C., Frenk, C., Blain, A., …Hainline, L. (2008). The properties of submm galaxies in hierarchical models. Monthly Notices of the Royal Astronomical Society, 391(1), 420-434. https://doi.org/10.1111/j.1365-2966.2008.13911.x

We use the combined GALFORM semi-analytical model of galaxy formation and GRASIL spectrophotometric code to investigate the properties of galaxies selected via their submillimetre (submm) emission. The fiducial model we use has previously been shown... Read More about The properties of submm galaxies in hierarchical models.

Erratum: ''deep Australia Telescope Large Area Survey Radio Observations of the European Large Area ISO Survey S1/SPITZER Wide-Area Infrared Extragalactic Field'' (2008, AJ, 135, 1276) (2008)
Journal Article
Middelberg, E., Norris, R., Cornwell, T., Voronkov, M., Siana, B., Boyle, B., …Smail, I. (2008). Erratum: ''deep Australia Telescope Large Area Survey Radio Observations of the European Large Area ISO Survey S1/SPITZER Wide-Area Infrared Extragalactic Field'' (2008, AJ, 135, 1276). Astronomical Journal, 136, 519-+. https://doi.org/10.1088/0004-6256/136/1/519

The SCUBA Half-Degree Extragalactic Survey (SHADES) - VIII. The nature of faint submillimetre galaxies in SHADES, SWIRE and SXDF surveys (2008)
Journal Article
Clements, D., Vaccari, M., Babbedge, T., Oliver, S., Rowan-Robinson, M., Davoodi, P., …van Kampen, E. (2008). The SCUBA Half-Degree Extragalactic Survey (SHADES) - VIII. The nature of faint submillimetre galaxies in SHADES, SWIRE and SXDF surveys. Monthly Notices of the Royal Astronomical Society, 387, 247-267. https://doi.org/10.1111/j.1365-2966.2008.13172.x

Weighing the black holes in z ~ 2 submillimeter-emitting galaxies hosting active galactic nuclei (2008)
Journal Article
Alexander, D., Brandt, W., Smail, I., Swinbank, A., Bauer, F., Blain, A., …Menéndez-Delmestre, K. (2008). Weighing the black holes in z ~ 2 submillimeter-emitting galaxies hosting active galactic nuclei. Astronomical Journal, 135(5), 1968-1981. https://doi.org/10.1088/0004-6256/135/5/1968

We place direct observational constraints on the black-hole masses (M BH) of the cosmologically important z≈ 2 submillimeter-emitting galaxy (SMG; f 850 μm gsim 4 mJy) population, and use measured host-galaxy masses to explore their evolutionary stat... Read More about Weighing the black holes in z ~ 2 submillimeter-emitting galaxies hosting active galactic nuclei.

Deep Australia Telescope Large Area Survey Radio Observations of the European Large Area ISO Survey S1/Spitzer Wide-Area Infrared Extragalactic Field (2008)
Journal Article
Middelberg, E., Norris, R., Cornwell, T., Voronkov, M., Siana, B., Boyle, B., …Smail, I. (2008). Deep Australia Telescope Large Area Survey Radio Observations of the European Large Area ISO Survey S1/Spitzer Wide-Area Infrared Extragalactic Field. Astronomical Journal, 135, 1276-1290. https://doi.org/10.1088/0004-6256/135/4/1276

The SCUBA HAlf Degree Extragalactic Survey - VI. 350-μm mapping of submillimetre galaxies (2008)
Journal Article
Coppin, K., Halpern, M., Scott, D., Borys, C., Dunlop, J., Dunne, L., …Vaccari, M. (2008). The SCUBA HAlf Degree Extragalactic Survey - VI. 350-μm mapping of submillimetre galaxies. Monthly Notices of the Royal Astronomical Society, 384(4), 1597-1610. https://doi.org/10.1111/j.1365-2966.2007.12808.x

A follow-up survey using the Submillimetre High-Angular Resolution Camera (SHARC-II) at 350 μm has been carried out to map the regions around several 850-μm-selected sources from the Submillimetre HAlf Degree Extragalactic Survey (SHADES). These obse... Read More about The SCUBA HAlf Degree Extragalactic Survey - VI. 350-μm mapping of submillimetre galaxies.

The SCUBA HAlf Degree Extragalactic Survey (SHADES) - V. Submillimetre properties of near-infrared-selected galaxies in the Subaru/XMM -Newton deep field (2007)
Journal Article
Takagi, T., Mortier, A., Shimasaku, K., Coppin, K., Pope, A., Ivison, R., …Vaccari, M. (2007). The SCUBA HAlf Degree Extragalactic Survey (SHADES) - V. Submillimetre properties of near-infrared-selected galaxies in the Subaru/XMM -Newton deep field. Monthly Notices of the Royal Astronomical Society, 381, 1154-1168. https://doi.org/10.1111/j.1365-2966.2007.12302.x

The evolution of the near-infrared galaxy luminosity function and colour bimodality up to z \~= 2 from the UKIDSS Ultra Deep Survey Early Data Release (2007)
Journal Article
Cirasuolo, M., McLure, R., Dunlop, J., Almaini, O., Foucaud, S., Smail, I., …Hirst, P. (2007). The evolution of the near-infrared galaxy luminosity function and colour bimodality up to z \~= 2 from the UKIDSS Ultra Deep Survey Early Data Release. Monthly Notices of the Royal Astronomical Society, 380, 585-595. https://doi.org/10.1111/j.1365-2966.2007.12038.x

A Detailed Study of Gas and Star Formation in a Highly Magnified Lyman Break Galaxy at z = 3.07 (2007)
Journal Article
Coppin, K., Swinbank, A., Neri, R., Cox, P., Smail, I., Ellis, R., …Richard, J. (2007). A Detailed Study of Gas and Star Formation in a Highly Magnified Lyman Break Galaxy at z = 3.07. Astrophysical Journal, 665(2), 936-943. https://doi.org/10.1086/519789

We report the detection of CO(3-2) emission from a bright, gravitationally lensed Lyman Break galaxy, LBG J213512.73-010143 (the "Cosmic Eye"), at z = 3.07, using the Plateau de Bure Interferometer. This is only the second detection of molecular gas... Read More about A Detailed Study of Gas and Star Formation in a Highly Magnified Lyman Break Galaxy at z = 3.07.

A CFH12k lensing survey of X-ray luminous galaxy clusters II : weak lensing analysis and global correlations (2007)
Journal Article
Bardeau, S., Soucail, G., Kneib, J., Czoske, O., Ebeling, H., Hudelot, P., …Smith, G. (2007). A CFH12k lensing survey of X-ray luminous galaxy clusters II : weak lensing analysis and global correlations. Astronomy & Astrophysics, 470(2), 449-466. https://doi.org/10.1051/0004-6361%3A20077443

Aims: We present a wide-field multi-color survey of a homogeneous sample of eleven clusters of galaxies for which we measure total masses and mass distributions from weak lensing. This sample, spanning a small range in both X-ray luminosity and redsh... Read More about A CFH12k lensing survey of X-ray luminous galaxy clusters II : weak lensing analysis and global correlations.

AEGIS20: A radio survey of the Extended Groth Strip (2007)
Journal Article
Ivison, R., Chapman, S., Faber, S., Smail, I., Biggs, A., Conselice, C., …Willner, S. (2007). AEGIS20: A radio survey of the Extended Groth Strip. Astrophysical Journal, 660(1), L77-L80

An Increase in the Faint Red Galaxy Population in Massive Clusters since z \~ 0.5 (2007)
Journal Article
Stott, J., Smail, I., Edge, A., Ebeling, H., Smith, G., Kneib, J., & Pimbblet, K. (2007). An Increase in the Faint Red Galaxy Population in Massive Clusters since z \~ 0.5. Astrophysical Journal, 661(1), 95-101. https://doi.org/10.1086/514329

We compare the luminosity functions for red galaxies lying on the rest-frame (U - V) color-magnitude sequence in a homogeneous sample of 10 X-ray-luminous clusters from the MACS survey at z ~ 0.5 to a similarly selected X-ray cluster sample at z ~ 0.... Read More about An Increase in the Faint Red Galaxy Population in Massive Clusters since z \~ 0.5.

Extending the infrared radio correlation (2007)
Journal Article
Boyle, B., Cornwell, T., Middelberg, E., Norris, R., Appleton, P., & Smail, I. (2007). Extending the infrared radio correlation. Monthly Notices of the Royal Astronomical Society, 376(3), 1182-1188

Resolved spectroscopy of a gravitationally lensed L* Lyman-break galaxy at z∼ 5. (2007)
Journal Article
Swinbank, A., Bower, R., Smith, G. P., Wilman, R., Smail, I., Ellis, R., …Kneib, J. (2007). Resolved spectroscopy of a gravitationally lensed L* Lyman-break galaxy at z∼ 5. Monthly Notices of the Royal Astronomical Society, 376(2), 479-491. https://doi.org/10.1111/j.1365-2966.2007.11454.x

We exploit the gravitational potential of a massive, rich cluster at z= 0.77 to study the internal properties of a gravitationally lensed galaxy at z= 4.88. Using high-resolution Hubble Space Telescope imaging together with optical (VIMOS) and near-i... Read More about Resolved spectroscopy of a gravitationally lensed L* Lyman-break galaxy at z∼ 5..

A Very Bright, Highly Magnified Lyman Break Galaxy at z = 3.07. (2007)
Journal Article
Smail, I., Swinbank, A., Richard, J., Ebeling, H., Kneib, J., Edge, A., …Mullis, C. (2007). A Very Bright, Highly Magnified Lyman Break Galaxy at z = 3.07. Astrophysical Journal Letters, 654(1), L33-L36. https://doi.org/10.1086/510902

Using Hubble Space Telescope imaging and Keck spectroscopy, we report the discovery of a very bright, highly magnified (~30 times) Lyman break galaxy (LBG) at z = 3.07 in the field of the massive z = 0.33 cluster MACS J2135.2-0102. The system compris... Read More about A Very Bright, Highly Magnified Lyman Break Galaxy at z = 3.07..

Truncation of galaxy dark matter halos in high density environments (2007)
Journal Article
Limousin, M., Kneib, J., Bardeau, S., Natarajan, P., Czoske, O., Smail, I., …Smith, G. (2007). Truncation of galaxy dark matter halos in high density environments. Astronomy & Astrophysics, 461(3), 881-891. https://doi.org/10.1051/0004-6361%3A20065543

Aims: Our aim is to constrain the properties of dark matter halos inhabiting high density environments, such as is the case in massive galaxy clusters. Methods: We use galaxy-galaxy lensing techniques that utilize a maximum likelihood method to const... Read More about Truncation of galaxy dark matter halos in high density environments.

The 2dF-SDSS LRG and QSO Survey: the star formation histories of luminous red galaxies. (2006)
Journal Article
Roseboom, I., Pimbblet, K., Drinkwater, M., Cannon, R., de Propris, R., Edge, A., …Weilbacher, P. (2006). The 2dF-SDSS LRG and QSO Survey: the star formation histories of luminous red galaxies. Monthly Notices of the Royal Astronomical Society, 373(1), 349-360. https://doi.org/10.1111/j.1365-2966.2006.11024.x

We present a detailed investigation into the recent star formation histories of 5697 luminous red galaxies (LRGs) based on the Hδ (4101 Å), and [O II] (3727 Å) lines and the D4000 index. LRGs are luminous (L > 3L*) galaxies which have been selected t... Read More about The 2dF-SDSS LRG and QSO Survey: the star formation histories of luminous red galaxies..

The SCUBA half-degree extragalactic survey - II. Submillimetre maps, catalogue and number counts (2006)
Journal Article
Coppin, K., Chapin, E., Mortier, A., Scott, S., Borys, C., Dunlop, J., …Willott, C. (2006). The SCUBA half-degree extragalactic survey - II. Submillimetre maps, catalogue and number counts. Monthly Notices of the Royal Astronomical Society, 372(4), 1621-1652. https://doi.org/10.1111/j.1365-2966.2006.10961.x

We present maps, source catalogue and number counts of the largest, most complete and unbiased extragalactic submillimetre survey: the 850-μm SCUBA Half-Degree Extragalactic Survey (SHADES). Using the Submillimetre Common-User Bolometer Array (SCUBA)... Read More about The SCUBA half-degree extragalactic survey - II. Submillimetre maps, catalogue and number counts.

The 2df SDSS LRG and QSO survey: evolution of the luminosity function of luminous red galaxies to z= 0.6 (2006)
Journal Article
Wake, D., Nichol, R., Eisenstein, D., Loveday, J., Edge, A., Cannon, R., …Brinkmann, J. (2006). The 2df SDSS LRG and QSO survey: evolution of the luminosity function of luminous red galaxies to z= 0.6. Monthly Notices of the Royal Astronomical Society, 372(2), 537-550. https://doi.org/10.1111/j.1365-2966.2006.10831.x

We present new measurements of the luminosity function (LF) of luminous red galaxies (LRGs) from the Sloan Digital Sky Survey (SDSS) and the 2dF SDSS LRG and Quasar (2SLAQ) survey. We have carefully quantified, and corrected for, uncertainties in the... Read More about The 2df SDSS LRG and QSO survey: evolution of the luminosity function of luminous red galaxies to z= 0.6.

A panoramic mid-infrared survey of two distant clusters (2006)
Journal Article
Geach, J., Smail, I., Ellis, R., Moran, S., Smith, G., Treu, T., …Kodama, T. (2006). A panoramic mid-infrared survey of two distant clusters. Astrophysical Journal, 649(2), 661-672. https://doi.org/10.1086/506469

We present panoramic Spitzer MIPS 24 μm observations, covering ~9 × 9 Mpc2 (25' × 25') fields around two massive clusters, Cl 0024+16 and MS 0451-03, at z = 0.39 and z = 0.55, respectively, reaching a 5 σ flux limit of ~200 μJy. Our observations cove... Read More about A panoramic mid-infrared survey of two distant clusters.

The X-ray spectral properties of scuba galaxies (2005)
Journal Article
Alexander, D., Bauer, F., Chapman, S., Smail, I., Blain, A., Brandt, W., & Ivison, R. (2005). The X-ray spectral properties of scuba galaxies. Astrophysical Journal, 632(2), 736-750. https://doi.org/10.1086/444342

Deep SCUBA surveys have uncovered a large population of massive submillimeter-emitting galaxies (SMGs; f850m 4 mJy) at z 1. Although it is generally believed that these galaxies host intense star formation activity, there is growing evidence that a s... Read More about The X-ray spectral properties of scuba galaxies.

A Hubble space telescope lensing survey of X-ray luminous galaxy clusters - IV. Mass, structure and thermodynamics of cluster cores at z= 0.2 (2005)
Journal Article
Smith, G., Kneib, J., Smail, I., Mazzotta, P., Ebeling, H., & Czoske, O. (2005). A Hubble space telescope lensing survey of X-ray luminous galaxy clusters - IV. Mass, structure and thermodynamics of cluster cores at z= 0.2. Monthly Notices of the Royal Astronomical Society, 359(2), 417-446. https://doi.org/10.1111/j.1365-2966.2005.08911.x

We present a comprehensive space-based study of 10 X-ray luminous galaxy clusters (LX>= 8 × 1044 erg s-1, 0.1-2.4 keV) at z= 0.2. Hubble Space Telescope (HST) observations reveal numerous gravitationally lensed arcs for which we present four new spec... Read More about A Hubble space telescope lensing survey of X-ray luminous galaxy clusters - IV. Mass, structure and thermodynamics of cluster cores at z= 0.2.

Molecular gas in a z ∼ 2.5 triply-imaged, sub-mJy submillimetre galaxy typical of the cosmic far-infrared background (2005)
Journal Article
Kneib, J., Neri, R., Smail, I., Blain, A., Sheth, K., van der Werf, P., & Knudsen, K. (2005). Molecular gas in a z ∼ 2.5 triply-imaged, sub-mJy submillimetre galaxy typical of the cosmic far-infrared background. Astronomy & Astrophysics, 434(3), 819-825. https://doi.org/10.1051/0004-6361%3A20042034

We present the results of observations from the Plateau de Bure IRAM interferometric array of the submillimetre (submm) galaxy SMMJ16359+6612 lying at z = 2.516 behind the core of the massive cluster A2218. The foreground gravitational lens produces... Read More about Molecular gas in a z ∼ 2.5 triply-imaged, sub-mJy submillimetre galaxy typical of the cosmic far-infrared background.

A CFH12k lensing survey of X-ray luminous galaxy clusters I : weak lensing methodology (2005)
Journal Article
Bardeau, S., Kneib, J., Czoske, O., Soucail, G., Smail, I., Ebeling, H., & Smith, G. (2005). A CFH12k lensing survey of X-ray luminous galaxy clusters I : weak lensing methodology. Astronomy & Astrophysics, 434(2), 433-448. https://doi.org/10.1051/0004-6361%3A20041643

We describe the weak lensing methodology we have applied to multi-colour CFH12k imaging of a homogeneouslyselected sample of luminous X-ray clusters at z ∼ 0.2. The aim of our survey is to understand the variation in cluster structure and dark matter... Read More about A CFH12k lensing survey of X-ray luminous galaxy clusters I : weak lensing methodology.

An ISOCAM survey through gravitationally lensing galaxy clusters III : new results from mid-infrared observations of the cluster Abell 2219 (2005)
Journal Article
Coia, D., Metcalfe, L., McBreen, B., Biviano, A., Smail, I., Altieri, B., …O'Halloran, B. (2005). An ISOCAM survey through gravitationally lensing galaxy clusters III : new results from mid-infrared observations of the cluster Abell 2219. Astronomy & Astrophysics, 430(1), 59-66. https://doi.org/10.1051/0004-6361%3A20041648

The massive cluster of galaxies Abell 2219 (z = 0.228) with two spectacular gravitational lensing arcs was observed at 14.3 μm (hereafter 15 μm) with the Infrared Space Observatory and results were published by Barvainis et al. (\cite{1999AJ....118..... Read More about An ISOCAM survey through gravitationally lensing galaxy clusters III : new results from mid-infrared observations of the cluster Abell 2219.

The rest-frame optical properties of SCUBA galaxies (2004)
Journal Article
Smail, I., Chapman, S., Blain, A., & Ivison, R. (2004). The rest-frame optical properties of SCUBA galaxies. Astrophysical Journal, 616(1), 71-85. https://doi.org/10.1086/424896

We present optical and near-infrared photometry for a sample of 96 dusty, far-infraredluminous galaxies. We have precise spectroscopic redshifts for all these galaxies, yielding a median redshift of = 2.2. The majority, 78, are submillimeter-detected... Read More about The rest-frame optical properties of SCUBA galaxies.

A vigorous starburst in the SCUBA galaxy N2 850.4 (2003)
Journal Article
Smail, I., Chapman, S., Ivison, R., Blain, A., Takata, T., Heckman, T., …Sekiguchi, K. (2003). A vigorous starburst in the SCUBA galaxy N2 850.4. Monthly Notices of the Royal Astronomical Society, 342, 1185-1193

Chandra Detections of SCUBA Galaxies around High-z Radio Sources. (2003)
Journal Article
Smail, I., Scharf, C., Ivison, R., Stevens, J., Bower, R., & Dunlop, J. (2003). Chandra Detections of SCUBA Galaxies around High-z Radio Sources. Astrophysical Journal, 599(1), 86-91. https://doi.org/10.1086/379233

The most massive galaxies in the present-day universe are the giant elliptical galaxies found in the centers of rich clusters. These have old, coeval stellar populations, suggesting they formed at high redshift, and are expected to host supermassive... Read More about Chandra Detections of SCUBA Galaxies around High-z Radio Sources..

The nature of X-ray selected extremely red objects (2003)
Journal Article
Stevens, J., Page, M., Ivison, R., Smail, I., Lehmann, I., Hasinger, G., & Szokoly, G. (2003). The nature of X-ray selected extremely red objects. Monthly Notices of the Royal Astronomical Society, 342, 249-258

INGRID: A near-infrared camera for the William Herschel Telescope (2003)
Journal Article
Packham, C., Thompson, K. L., Zurita, A., Knapen, J. H., Smail, I., Greimel, R., …Worswick, S. (2003). INGRID: A near-infrared camera for the William Herschel Telescope. Monthly Notices of the Royal Astronomical Society, 345, 395-405

The morphology-density relation in the Sloan Digital Sky Survey (2003)
Journal Article
Goto, T., Yamauchi, C., Fujita, Y., Okamura, S., Sekiguchi, M., Smail, I., …Gomez, P. L. (2003). The morphology-density relation in the Sloan Digital Sky Survey. Monthly Notices of the Royal Astronomical Society, 346, 601-614

Measuring σ₈ with Cluster Lensing: Biases from Unrelaxed Clusters. (2003)
Journal Article
Smith, G. P., Edge, A. C., Eke, V. R., Nichol, R. C., Smail, I., & Kneib, J. (2003). Measuring σ₈ with Cluster Lensing: Biases from Unrelaxed Clusters. Astrophysical Journal, 590(2), L79-L82. https://doi.org/10.1086/376747

We use gravitational lens models and X-ray spectral analysis of 10 X-ray-luminous galaxy clusters at z sime 0.2 to study the impact of cluster substructure on attempts to normalize the matter power spectrum. We estimate that unrelaxed clusters are 30... Read More about Measuring σ₈ with Cluster Lensing: Biases from Unrelaxed Clusters..

A median redshift of 2.4 for galaxies bright at submillimetre wavelengths (2003)
Journal Article
Chapman, S., Blain, A., Ivison, R., & Smail, I. (2003). A median redshift of 2.4 for galaxies bright at submillimetre wavelengths. Nature, 422(6933), 695-698. https://doi.org/10.1038/nature01540

A significant fraction of the energy emitted in the early Universe came from very luminous galaxies that are largely hidden at optical wavelengths (because of interstellar dust grains); this energy now forms part of the cosmic background radiation at... Read More about A median redshift of 2.4 for galaxies bright at submillimetre wavelengths.

An Hα survey of the rich cluster A 1689 (2002)
Journal Article
Balogh, M. L., Couch, W. J., Smail, I., Bower, R. G., & Glazebrook, K. (2002). An Hα survey of the rich cluster A 1689. Monthly Notices of the Royal Astronomical Society, 335, 10-22

The dark side of galaxy formation (2002)
Journal Article
Smail, I. (2002). The dark side of galaxy formation. Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences, 360, 2697-2710

Submillimeter galaxies (2002)
Journal Article
Blain, A. W., Smail, I., Ivison, R., Kneib, J., & Frayer, D. T. (2002). Submillimeter galaxies. Physics Reports, 369, 111-176

The Diversity of Extremely Red Objects (2002)
Journal Article
Smail, I., Owen, F., Morrison, G., Keel, W., Ivison, R., & Ledlow, M. (2002). The Diversity of Extremely Red Objects. Astrophysical Journal, 581, 844-864

The nature of faint submillimetre-selected galaxies (2002)
Journal Article
Smail, I., Ivison, R., Blain, A., & Kneib, J. (2002). The nature of faint submillimetre-selected galaxies. Monthly Notices of the Royal Astronomical Society, 331(2), 495-520. https://doi.org/10.1046/j.1365-8711.2002.05203.x

We present the source catalogue for the SCUBA Lens Survey. We summarize the results of extensive multiwavelength observations of the 15 submillimetre-selected galaxies in the catalogue, from X-rays to radio. We discuss the main observational characte... Read More about The nature of faint submillimetre-selected galaxies.

Distinguishing Local and Global Influences on Galaxy Morphology: A Hubble Space Telescope Comparison of High and Low X-Ray Luminosity Clusters. (2002)
Journal Article
Balogh, M. L., Smail, I., Bower, R., Ziegler, B., Smith, G., Davies, R. L., …Ebeling, H. (2002). Distinguishing Local and Global Influences on Galaxy Morphology: A Hubble Space Telescope Comparison of High and Low X-Ray Luminosity Clusters. Astrophysical Journal, 566(1), 123-136. https://doi.org/10.1086/338056

We present a morphological analysis of 17 X-ray-selected clusters at z ~ 0.25, imaged uniformly with the Hubble Space Telescope Wide Field Planetary Camera 2 (WFPC2). Eight of these clusters comprise a subsample selected for their low X-ray luminosit... Read More about Distinguishing Local and Global Influences on Galaxy Morphology: A Hubble Space Telescope Comparison of High and Low X-Ray Luminosity Clusters..

VLT spectroscopy of galaxies lensed by the AC 114 cluster : implications for the mass model and the study of low-luminosity galaxies at high-redshift (2001)
Journal Article
Campusano, L., Pelló, R., Kneib, J., Le Borgne, J., Fort, B., Ellis, R., …Smail, I. (2001). VLT spectroscopy of galaxies lensed by the AC 114 cluster : implications for the mass model and the study of low-luminosity galaxies at high-redshift. Astronomy & Astrophysics, 378(2), 394-407. https://doi.org/10.1051/0004-6361%3A20011216

We present the first results of a spectroscopic survey of faint lensed galaxies in the core of the galaxy cluster AC 114 (z=0.312) obtained from observations with the FORS1 spectrograph mounted on the VLT-Antu (Unit Telescope 1). The galaxies were ch... Read More about VLT spectroscopy of galaxies lensed by the AC 114 cluster : implications for the mass model and the study of low-luminosity galaxies at high-redshift.

The early-type galaxy population in Abell 2218 (2001)
Journal Article
Ziegler, B. L., Bower, R. G., Smail, I., Davies, R. L., & Lee, D. (2001). The early-type galaxy population in Abell 2218. Monthly Notices of the Royal Astronomical Society, 325(4), 1571-1590. https://doi.org/10.1046/j.1365-8711.2001.04563.x

We present high signal-to-noise, moderate-resolution spectroscopy of 48 early-type members of the rich cluster Abell 2218 at z = 0.18, taken with the LDSS2 spectrograph on the 4.2-m William Herschel Telescope. This sample both is larger and spans a w... Read More about The early-type galaxy population in Abell 2218.

The optical afterglow and host galaxy of GRB 000926 (2001)
Journal Article
Fynbo, J., Gorosabel, J., Dall, T., Hjorth, J., Pedersen, H., Andersen, M., …Terada, H. (2001). The optical afterglow and host galaxy of GRB 000926. Astronomy & Astrophysics, 373(3), 796-804. https://doi.org/10.1051/0004-6361%3A20010531

We present the discovery of the Optical Transient (OT) of the long-duration gamma-ray burst GRB 000926. The optical transient was detected independently with the Nordic Optical Telescope and at Calar Alto 22.2 hours after the burst. At this time the... Read More about The optical afterglow and host galaxy of GRB 000926.

The diversity of SCUBA-selected galaxies (2000)
Journal Article
Ivison, R., Smail, I., Barger, A., Kneib, J., Blain, A., Owen, F., …Cowie, L. (2000). The diversity of SCUBA-selected galaxies. Monthly Notices of the Royal Astronomical Society, 315, 209-222

Deep Counts of Submillimeter Galaxies (1999)
Journal Article
Blain, A., Kneib, J., Ivison, R., & Smail, I. (1999). Deep Counts of Submillimeter Galaxies. Astrophysical Journal, 512, L87-L90

The history of star formation in dusty galaxies (1999)
Journal Article
Blain, A., Smail, I., Ivison, R., & Kneib, J. (1999). The history of star formation in dusty galaxies. Monthly Notices of the Royal Astronomical Society, 302, 632-648

Counts and colours of faint galaxies in the U and R bands (1997)
Journal Article
Hogg, D. W., Pahre, M. A., McCarthy, J. K., Cohen, J. G., Blandford, R., Smail, I., & Soifer, B. (1997). Counts and colours of faint galaxies in the U and R bands. Monthly Notices of the Royal Astronomical Society, 288, 404-410

Weak Gravitational Lensing by Galaxies (1996)
Journal Article
Brainerd, T. G., Blandford, R. D., & Smail, I. (1996). Weak Gravitational Lensing by Galaxies. Astrophysical Journal, 466, 623-

The life-cycle of star formation in distant clusters (1996)
Journal Article
Barger, A., Aragon-Salamanca, A., Ellis, R., Couch, W., Smail, I., & Sharples, R. (1996). The life-cycle of star formation in distant clusters. Monthly Notices of the Royal Astronomical Society, 279, 1-24

The Nature of Star Formation in Lensed Galaxies at High Redshift (1993)
Journal Article
Smail, I., Ellis, R., Aragón-Salamanca, A., Soucail, G., Mellier, Y., & Giraud, E. (1993). The Nature of Star Formation in Lensed Galaxies at High Redshift. Monthly Notices of the Royal Astronomical Society, 263(3), 628-640. https://doi.org/10.1093/mnras/263.3.628

We present near-infrared photometry of all available gravitationally lensed ‘arcs’ with spectroscopic redshifts. By combining this photometry with optical data, we find that the bulk of the systems with z ~ 1 are intrinsically blue across the rest-fr... Read More about The Nature of Star Formation in Lensed Galaxies at High Redshift.

A statistically complete survey for arc-like features in images of distant rich clusters of galaxies (1991)
Journal Article
Smail, I., Ellis, R., Fitchett, M., Nørgaard-Nielsen, H., Hansen, L., & Jørgensen, H. (1991). A statistically complete survey for arc-like features in images of distant rich clusters of galaxies. Monthly Notices of the Royal Astronomical Society, 252(1), 19-29. https://doi.org/10.1093/mnras/252.1.19

Using data from an earlier search for supernovae in distant clusters, we have constructed a homogeneous set of V images for 19 rich clusters with mean redshift z¯¯¯=0.32z¯=0.32. By considering the images above a fixed surface brightness limit, the da... Read More about A statistically complete survey for arc-like features in images of distant rich clusters of galaxies.

Spectroscopy of arcs in the rich cluster Abell 963 (1991)
Journal Article
Ellis, R., Allington-Smith, J., & Smail, I. (1991). Spectroscopy of arcs in the rich cluster Abell 963. Monthly Notices of the Royal Astronomical Society, 249(1), 184-190. https://doi.org/10.1093/mnras/249.1.184

Spectra are presented for portions of the two arcs observed close to the dominant cD galaxy in the rich cluster Abell 963 (z = 0.206). The spectrum of the northern arc displays a strong emission line at 6600 Å which is seen along the entire arc. The... Read More about Spectroscopy of arcs in the rich cluster Abell 963.