Understanding the properties of dust attenuation curves in galaxies and the physical
mechanisms that shape them are among the fundamental questions of extragalactic …

Context. Measuring how the physical properties of galaxies change across cosmic times is
essential to understand galaxy formation and evolution. With the advent of numerous ground …

We make use of sensitive (9.3 μJy beam− 1 rms) 1.2 mm continuum observations from the
Atacama Large Millimeter/submillimeter Array (ALMA) Spectroscopic Survey in the Hubble …

We use a newly assembled sample of 3545 star-forming galaxies with secure spectroscopic,
grism, and photometric redshifts at z= 1.5–2.5 to constrain the relationship between UV …

We make use of deep 1.2 mm continuum observations (12.7 μJy beam− 1 rms) of a 1 arcmin
2 region in the Hubble Ultra Deep Field to probe dust-enshrouded star formation from 330 …

Star formation rate (SFR) measurements at z> 4 have relied mostly on the rest-frame far-
ultraviolet (FUV) observations. The corrections for dust attenuation based on the IRX-β …

We present dust attenuation properties of spectroscopically confirmed star forming galaxies
on the main sequence at a redshift of∼ 4.4− 5.8. Our analyses are based on the far infrared …

Context. Deep far-infrared (FIR) cosmological surveys are known to be affected by source
confusion, causing issues when examining the main sequence (MS) of star forming …

We make use of Atacama Large Millimeter/submillimeter Array continuum observations of 15
luminous Lyman-break galaxies at z∼ 7–8 to probe their dust-obscured star formation …

In recent years, observations have uncovered a population of massive galaxies that are
invisible or very faint in deep optical/near-infrared (near-IR) surveys but brighter at longer …