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20132024
most citedLOFAR/H-ATLAS: The low-frequency radio luminosity - star-formation rate relation

185 citations · 1.1k across the 20 of their papers we have counts for

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Showing astro-ph.GAShow all

30 papers · 1 filter

astro-ph.GA202414 cited

The fate of the interstellar medium in early-type galaxies. III. The mechanism of ISM removal and quenching of star formation

Michał J. Michałowski, C. Gall, J. Hjorth +15

Understanding how galaxies quench their star formation is crucial for studies of galaxy evolution. Quenching is related to the cold gas decrease. In the first paper we showed that…

astro-ph.GA2019109 cited

The East Asian Observatory SCUBA--2 survey of the COSMOS field: unveiling 1147 bright sub-millimeter sources across 2.6 square degrees

J. M. Simpson, Ian Smail, A. M. Swinbank +28

We present sensitive 850m imaging of the COSMOS field using 640hr of new and archival observations taken with SCUBA-2 at the East Asian Observatory's James Clerk Maxwell Telesco…

astro-ph.GA201933 cited

The fate of the interstellar medium in early-type galaxies. I. First direct measurement of the timescale of dust removal

Michał J. Michałowski, J. Hjorth, C. Gall +12

An important aspect of quenching star formation is the removal of the cold interstellar medium (ISM; non-ionised gas and dust) from a galaxy. In addition, dust grains can be destro…

astro-ph.GA201928 cited

Multi-wavelength properties of radio and machine-learning identified counterparts to submillimeter sources in S2COSMOS

FangXia An, J. M. Simpson, Ian Smail +36

We identify multi-wavelength counterparts to 1,147 submillimeter sources from the S2COSMOS SCUBA-2 survey of the COSMOS field by employing a recently developed radiomachine-lear…

astro-ph.GA2018

ALMA observations of massive molecular gas reservoirs in dusty early-type galaxies

A. E. Sansom, D. H. W. Glass, G. J. Bendo +9

Unresolved gas and dust observations show a surprising diversity in the amount of interstellar matter in early-type galaxies. Using ALMA observations we resolve the ISM in z0…

astro-ph.GA2018

The relationship between dust and [CI] at z=1 and beyond

N. Bourne, J. S. Dunlop, J. M. Simpson +3

Measuring molecular gas mass is vital for understanding the evolution of galaxies at high redshifts (z1). Most measurements rely on CO as a tracer, but dependences on metalli…