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

Lyman-break galaxy (LBG) candidates at z≳ 10 are rapidly being identified in James Webb
Space Telescope (JWST)/NIRCam observations. Due to the (redshifted) break produced by …

We report 18 dust continuum detections (≥ 3.3 σ) at∼ 88 and 158 out of 49 ultraviolet (UV)-
bright galaxies (M UV<− 21.3 mag) at> 6.5, observed by the Cycle-7 Atacama Large …

Context. Feedback from accreting supermassive black holes (SMBHs) is often identified as
the main mechanism responsible for regulating star formation in active galactic nucleus …

We combine molecular gas masses inferred from CO emission in 500 star-forming galaxies
(SFGs) between z= 0 and 3, from the IRAM-COLDGASS, PHIBSS1/2, and other surveys, with …

We compile observations of molecular gas contents and infrared-based star formation rates
(SFRs) for 112 circumnuclear star-forming regions, in order to reinvestigate the form of the …

We present results on the dust attenuation curve of z∼ 2 galaxies using early observations
from the MOSFIRE Deep Evolution Field survey. Our sample consists of 224 star-forming …

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 …

We present our new Atacama Large Millimeter/Submillimeter Array (ALMA) observations
targeting [O iii] 88 μm,[C ii] 158 μm,[N ii] 122 μm, and dust-continuum emission for three …

We present new calibrations of far-ultraviolet (FUV) attenuation as derived from the total
infrared to FUV luminosity ratio (IRX) and the FUV–near-UV (NUV) color. We find that the …