Outputs (518)

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.