129 citations · 460 across the 7 of their papers we have counts for
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An ALMA survey of the SCUBA-2 Cosmology Legacy SurveyUKIDSS/UDS Field: Halo Masses for Submillimetre Galaxies
S. M. Stach, I. Smail, A. Amvrosiadis +14
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-…
Massive molecular gas reservoir around the central AGN in the CARLA J1103+3449 cluster at z=1.44
Vladan Markov, Simona Mei, Philippe Salomé +14
Passive early-type galaxies dominate cluster cores at z 1.5. At higher redshift, cluster core galaxies are observed to have still on-going star-formation, fuelled by cold…
Extended H over compact far-infrared continuum in dusty submillimeter galaxies -- Insights into dust distributions and star-formation rates at
Chian-Chou Chen, C. M. Harrison, I. Smail +15
Using data from ALMA and near-infrared (NIR) integral field spectrographs including both SINFONI and KMOS on the VLT, we investigate the two-dimensional distributions of H and r…
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
B. Gullberg, I. Smail, A. M. Swinbank +15
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 S/N ratios of in high-r…
Revealing the Stellar Mass and Dust Distributions of Submillimeter Galaxies at Redshift 2
P. Lang, E. Schinnerer, Ian Smail +35
We combine high-resolution ALMA and HST/CANDELS observations of 20 submillimeter galaxies (SMGs) predominantly from the AS2UDS survey at z~2 with bright rest-frame optical counterp…
The submillimetre view of massive clusters at z~0.8-1.6
E. A. Cooke, Ian Smail, S. M. Stach +5
We analyse 850um 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 ove…