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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.

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.

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.

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.

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.

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.