609 citations · 2.5k across the 26 of their papers we have counts for
50 papers · 1 filter
Far-infrared observations of dust in Ly emitters at z=2-6
Rahul Rana, Julie L. Wardlow, Thomas M. Cornish +3
The bright Ly line is regularly used to identify high-redshift star-forming galaxies known as Ly emitters (LAEs). However, Ly is affected by resonant scattering and dust a…
The Radio Galaxy Environment Reference Survey (RAGERS): a submillimetre study of the environments of massive radio-quiet galaxies at
Thomas M. Cornish, Julie L. Wardlow, Thomas R. Greve +15
Measuring the environments of massive galaxies at high redshift is crucial to understanding galaxy evolution and the conditions that gave rise to the distribution of matter we see…
The RAdio Galaxy Environment Reference Survey (RAGERS): Evidence of an anisotropic distribution of submillimeter galaxies in the 4C 23.56 protocluster at z=2.48
Dazhi Zhou, Thomas R. Greve, Bitten Gullberg +41
High-redshift radio(-loud) galaxies (HRGs) are massive galaxies with powerful radio-loud active galactic nuclei (AGNs) and serve as beacons for protocluster identification. Howe…
An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field South: an unbiased study of SMG environments measured with narrowband imaging
Thomas M. Cornish, Julie Wardlow, Heather Wade +11
Submillimetre galaxies (SMGs) are some of the most extreme star-forming systems in the Universe, whose place in the framework of galaxy evolution is as yet uncertain. It has been h…
Bright beacons? ALMA non-detection of a supposedly bright [OI] 63-um line in a redshift-6 dusty galaxy
M. Rybak, L. Lemsom, A. Lundgren +8
We report a non-detection of the [OI] 63-um emission line from the z = 6.03 galaxy G09.83808 using ALMA Band 9 observations, refuting the previously claimed detection with APEX by…
KAOSS: turbulent, but disc-like kinematics in dust-obscured star-forming galaxies at 1.3-2.6
Jack E. Birkin, A. Puglisi, A. M. Swinbank +13
We present spatially resolved kinematics of 27 ALMA-identified dust-obscured star-forming galaxies (DSFGs) at 1.3-2.6, as traced by H emission using VLT/KMOS near-infrare…