E. da Cunha

TL;DR: In this article, the authors show that the variations of specific star formation rates (sSFRs = SFR/M*) are driven by varying gas fractions and that the hardness of the radiation field, which is proportional to the dust-mass-weighted luminosity (L IR/M dust) and the primary parameter defining the shape of the IR spectral energy distribution, is equivalent to SFE/Z.

TL;DR: In this article, the spectral energy distributions (SEDs) of star-forming galaxies were derived using an energy balance technique to connect the emission from stellar populations, dust attenuation, and dust emission in a physically consistent way.

TL;DR: In this article, the authors exploit the Atacama Large Millimeter Array (ALMA) 870 mu m observations of sub-millimetre sources in the Extended Chandra Deep Field South (EDF South) to investigate the far-infrared properties of high-redshift sub millimetre galaxies (SMGs).

TL;DR: In this article, the authors presented the first photometric redshift distribution for a large sample of 870 mu m submillimeter galaxies (SMGs) with robust identifications based on observations with ALMA.

TL;DR: The first direct and unbiased measurement of the evolution of the dust mass function of galaxies over the past 5 billion years of cosmic history using data from the Science Demonstration Phase of the Herschel-Astrophysical Terahertz Large Area Survey (Herschel-ATLAS) is presented in this paper.