activity
20032024
most citedThe Herschel ATLAS

596 citations · 12.4k across the 194 of their papers we have counts for

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Showing 2018 · astro-ph.GAShow all

11 papers · 2 filters

astro-ph.GA2018★ 1 cited

The nature of the variable millimetre-selected AGN in the Brightest Cluster Galaxy of Abell 851

R. A. Cheale, J. E. Geach, A. C. Edge +2

We present the detection of a bright 3mm continuum source in the Brightest Cluster Galaxy (BCG) in Abell 851 (z=0.411) with the NOrthern Extended Millimeter Array (NOEMA). When thi…

astro-ph.GA2018★ 41 cited

Two sub-millimetre bright protoclusters bounding the epoch of peak star-formation activity

Kevin Lacaille, Scott Chapman, Ian Smail +8

We present James Clerk Maxwell Telescope Submillimetre Common-User Bolometer Array 2 (SCUBA-2) 850 & 450 m observations ( mJy, mJy) of the HS1549+…

astro-ph.GA2018★ 21 cited

Violent quenching: molecular gas blown to 1000 km/s during a major merger

J. E. Geach, C. Tremonti, A. M. Diamond-Stanic +7

We present Atacama Large Millimeter/submillimeter Array observations of a massive (M_stars~10^11 M_Sun) compact (r_e,UV~100 pc) merger remnant at z=0.66 that is driving a 1000 km/s…

astro-ph.GA2018★ 28 cited

A magnified view of circumnuclear star formation and feedback around an AGN at z=2.6

J. E. Geach, R. J. Ivison, S. Dye +1

We present Atacama Large Millimeter/submillimeter Array observations of a radio-loud and millimeter-bright galaxy at z=2.6. Gravitational lensing by a foreground galaxy at z~0.2 pr…

astro-ph.GA2018★ 36 cited

A machine-learning method for identifying multi-wavelength counterparts of submillimeter galaxies: training and testing using AS2UDS and ALESS

FangXia An, S. M. Stach, Ian Smail +23

We describe the application of the supervised machine-learning algorithms to identify the likely multi-wavelength counterparts to submillimeter sources detected in panoramic, singl…

astro-ph.GA2018★ 97 cited

An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: number counts of submillimeter galaxies

S. M. Stach, I. Smail, A. M. Swinbank +23

We report the first results of AS2UDS: an 870 m continuum survey with the Atacama Large Millimeter/Submillimeter Array (ALMA) of a total area of 50 arcmin comprising…

astro-ph.GA2018★ 98 cited

The dust and [CII] morphologies of redshift ~4.5 sub-millimeter galaxies at ~200pc resolution: The absence of large clumps in the interstellar medium of high-redshift galaxies

B. Gullberg, A. M. Swinbank, I. Smail +27

We present deep high resolution (0.03", 200pc) ALMA Band 7 observations covering the dust continuum and [CII] m emission in four sub-millimeter galaxi…

astro-ph.GA2018★ 32 cited

Observational constraints on the physical nature of submillimetre source multiplicity: chance projections are common

Christopher C. Hayward, Scott C. Chapman, Charles C. Steidel +19

Interferometric observations have demonstrated that a significant fraction of single-dish submillimetre (submm) sources are blends of multiple submm galaxies (SMGs), but the nature…

astro-ph.GA2018★ 25 cited

Red, redder, reddest: SCUBA-2 imaging of colour-selected \textit{Herschel} sources

S. Duivenvoorden, S. Oliver, J. M. Scudder +28

High-redshift, luminous, dusty star forming galaxies (DSFGs) constrain the extremity of galaxy formation theories. The most extreme are discovered through follow-up on candidates i…

astro-ph.GA2018★ 40 cited

The dependence of galaxy clustering on stellar mass, star-formation rate and redshift at z = 0.8-2.2, with HiZELS

R. K. Cochrane, P. N. Best, D. Sobral +3

The deep, near-infrared narrow-band survey HiZELS has yielded robust samples of H-alpha emitting star-forming galaxies within narrow redshift slices at z = 0.8, 1.47 and 2.23. In t…

astro-ph.GA2018★ 50 cited

A direct calibration of the IRX-β relation in Lyman-break Galaxies at z=3-5

M. P. Koprowski, K. E. K. Coppin, J. E. Geach +17

We use a sample of 4178 Lyman break galaxies (LBGs) at z = 3, 4 and 5 in the UKIRT Infrared Deep Sky Survey (UKIDSS) Ultra Deep Survey (UDS) field to investigate the relationship b…