activity
19972026
most citedA Deep Sub-millimeter Survey of Lensing Clusters: A New Window on Galaxy Formation and Evolution

1.2k citations · 40k across the 385 of their papers we have counts for

collaborators

368 papers

astro-ph.GA2026

Tracing Radio AGN-Driven Quenching in Post-Starburst Galaxies at Cosmic Noon

Pallavi Patil, Kate Rowlands, Katherine Alatalo +14

We present a radio continuum study of photometrically selected cosmic noon (0.5<z<3) post-starburst galaxies (PSBs) in the UKIDSS Deep Survey (UDS) field to assess if radio-mode Ac…

astro-ph.GA2025★ 1 cited

Resolved Schmidt-Kennicutt relation in a binary hyperluminous infrared galaxy at

Jonathan S. Gómez, Hugo Messias, Neil M. Nagar +3

Hyperluminous infrared galaxies (HyLIRGs; SFRs up to about 1000 Msun yr-1), though rare, provide key constraints on galaxy evolution. H-ATLAS J084933.4+021443, a z = 2.41 binary Hy…

astro-ph.GA2025

Serendipitous Discovery of an Optically-Dark Ultra-Luminous Infrared Galaxy at = 3.4

N. H. Hayatsu, Zhi-Yu Zhang, R. J. Ivison +10

Dusty, submillimeter-selected galaxies without optical counterparts contribute a non-negligible fraction of the star formation in the early universe. However, such a population is…

astro-ph.GA2025★ 1 cited

HerS-3: An Exceptional Einstein Cross Reveals a Massive Dark Matter Halo

P. Cox, K. M. Butler, C. R. Keeton +24

We present a study of HerS-3, a dusty star-forming galaxy at zspec = 3.0607, which is gravitationally amplified into an Einstein cross with a fifth image of the background galaxy s…

astro-ph.GA2025★ 5 cited

ALMACAL XIII. Evolution of the CO luminosity function and the molecular gas mass density out to ~ 6

Victoria Bollo, Céline Péroux, Martin Zwaan +7

Cold molecular gas, largely traced by CO emission, is the primary fuel for star formation, making it essential for understanding galaxy evolution. ALMA has made significant progres…

astro-ph.GA2024

A Novel high-z submm Galaxy Efficient Line Survey in ALMA bands 3 through 8 -- An ANGELS Pilot

T. J. L. C. Bakx, A. Amvrosiadis, G. J. Bendo +32

We use the Atacama Large sub/Millimetre Array (ALMA) to efficiently observe spectral lines across Bands 3, 4, 5, 6, 7, and 8 at high-resolution (0.5" - 0.1") for 16 bright southern…