Over the past two decades, an avalanche of new data from multiwavelength imaging and
spectroscopic surveys has revolutionized our view of galaxy formation and evolution. Here …

Fitting the spectral energy distributions (SEDs) of galaxies is an almost universally used
technique that has matured significantly in the last decade. Model predictions and fitting …

We study the dust attenuation curves of 230,000 individual galaxies in the local universe,
ranging from quiescent to intensely star-forming systems, using GALEX, SDSS, and WISE …

We present an analysis of the deepest Herschel images in four major extragalactic fields
GOODS–North, GOODS–South, UDS, and COSMOS obtained within the GOODS–Herschel …

The extragalactic background light (EBL) is of fundamental importance both for
understanding the entire process of galaxy evolution and for γ-ray astronomy, but the overall …

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 …

We measure the evolution of the stellar mass function (SMF) from z= 0–1 using multi-
wavelength imaging and spectroscopic redshifts from the PRism MUlti-object Survey …

Distant star-forming galaxies show a correlation between their star formation rates (SFRs)
and stellar masses, and this has deep implications for galaxy formation. Here, we present a …

Calculating the galaxy merger rate requires both a census of galaxies identified as merger
candidates and a cosmologically averaged" observability" timescale< T obs (z)> for …

In this paper, we present the GALEX–SDSS–WISE Legacy Catalog (GSWLC), a catalog of
physical properties (stellar masses, dust attenuations, and star formation rates [SFRs]) for∼ …