Far-infrared and submillimeter wavelength surveys have now established the important role
of dusty, star-forming galaxies (DSFGs) in the assembly of stellar mass and the evolution of …

In recent years, observations of the Sunyaev-Zeldovich (SZ) effect have had significant
cosmological implications and have begun to serve as a powerful and independent probe of …

ALMA observations of the long wavelength dust continuum are used to estimate the
interstellar medium (ISM) masses in a sample of 708 galaxies at z= 0.3 to 4.5 in the …

We present ALMA Band 9 observations of the [C ii] 158 m emission for a sample of 10 main-
sequence galaxies at redshift∼ 2, with typical stellar masses (log M⋆/M⊙∼ 10.0–10.9) and …

Abstract The Herschel Multi-tiered Extragalactic Survey (HerMES) is a legacy programme
designed to map a set of nested fields totalling∼ 380 deg2. Fields range in size from 0.01 …

Abstract We exploit Atacama Large Millimeter Array (ALMA) 870 μm observations of sub-
millimetre sources in the Extended Chandra Deep Field South to investigate the far-infrared …

We present a" super-deblended" far-infrared (FIR) to (sub) millimeter photometric catalog in
the Cosmic Evolution Survey (COSMOS), prepared with the method recently developed by …

Three billion years after the big bang (at redshift z= 2), half of the most massive galaxies
were already old, quiescent systems with little to no residual star formation and extremely …

We exploit the deep and extended far-IR data sets (at 70, 100 and 160 μm) of the Herschel
Guaranteed Time Observation (GTO) PACS Evolutionary Probe (PEP) Survey, in …

EMU is a wide-field radio continuum survey planned for the new Australian Square
Kilometre Array Pathfinder (ASKAP) telescope. The primary goal of EMU is to make a deep …