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The relationship between dust and [C I] at z = 1 and beyond
Measuring molecular gas mass is vital for understanding the evolution of galaxies at high redshifts (z ≳ 1). Most measurements rely on CO as a tracer, but dependencies on metallicity, dynamics, and surface density lead to ...
The SCUBA-2 Cosmology Legacy Survey: Multiwavelength Counterparts to 10$^3$ Submillimeter Galaxies in the UKIDSS-UDS Field
We present multiwavelength identifications for the counterparts of 1088 submillimeter sources detected at 850 μm in the SCUBA-2 Cosmology Legacy Survey study of the UKIRT Infrared Deep Sky Survey-Ultra-Deep Survey (UDS) ...