activity
20142024
most citedThe SCUBA-2 Cosmology Legacy Survey: 850um maps, catalogues and number counts

331 citations · 1.3k across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.GA2024

A Comparative Study of the Ground State Transitions of CO and [C I] as Molecular Gas Tracers at High Redshift

Marta Frias Castillo, Matus Rybak, Jacqueline A. Hodge +22

The CO(1--0) and [\ion{C}{1}](1--0) emission lines are well-established tracers of cold molecular gas mass in local galaxies. At high redshift, where the interstellar medium (ISM)…

astro-ph.CO2024

A Full Resolution of the 450 μm Extragalactic Background Light

Qi-Ning Hsu, L. L. Cowie, Chian-Chou Chen +1

The extragalactic background light (EBL) is the cumulative radiation outside the Milky Way. The determination of its corresponding primary emitting sources as well as its total ene…

astro-ph.CO20243 cited

Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: Surveying the distant Universe

Eelco van Kampen, Tom Bakx, Carlos De Breuck +27

During the most active period of star formation in galaxies, which occurs in the redshift range 1<z<3, strong bursts of star formation result in significant quantities of dust, whi…

astro-ph.GA20246 cited

Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: The hidden circumgalactic medium

Minju M. Lee, Alice Schimek, Claudia Cicone +29

Our knowledge of galaxy formation and evolution has incredibly progressed through multi-wavelength observational constraints of the interstellar medium (ISM) of galaxies at all cos…

astro-ph.GA20235 cited

MAGNIF: A Tentative Lensed Rotating Disk at detected by JWST NIRCam WFSS with Dynamical Forward Modeling

Zihao Li, Zheng Cai, Fengwu Sun +39

We report galaxy MACS0416-Y3 behind the lensing cluster MACSJ0416.1--2403 as a tentative rotating disk at detected through its [OIII] emission in JWST NIRCam…

astro-ph.GA2023

Submillimetre galaxies as laboratories for dust grain coagulation

Hiroyuki Hirashita, Chian-Chou Chen

Coagulation in the dense interstellar medium (ISM) is an important process that determines the size of the largest grains. We use submillimetre galaxies (SMGs) as laboratories of g…