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 …

The disks of disk galaxies contain a substantial fraction of their baryonic matter and angular
momentum, and much of the evolutionary activity in these galaxies, such as the formation of …

ABSTRACT The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey
(CANDELS) is designed to document the first third of galactic evolution, over the …

This paper describes the first catalogue of photometrically derived stellar mass estimates for
intermediate-redshift (z< 0.65; median z= 0.2) galaxies in the Galaxy And Mass Assembly …

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 …

The circumgalactic medium (CGM) is fed by galaxy outflows and accretion of intergalactic
gas, but its mass, heavy element enrichment, and relation to galaxy properties are poorly …

ABSTRACT The Sloan Digital Sky Survey (SDSS) started a new phase in 2008 August, with
new instrumentation and new surveys focused on Galactic structure and chemical evolution …

We present deep near-IR (NIR) medium-bandwidth photometry over the wavelength range 1–
1.8 μm in the All-wavelength Extended Groth strip International Survey (AEGIS) and Cosmic …

Galaxy–galaxy interactions are predicted to cause gas inflows leading to enhanced nuclear
star formation. This prediction is borne out observationally, and is also supported by the gas …

We report the discovery of a powerful molecular wind from the nucleus of the non-interacting
nearby S0 field galaxy NGC 1266. The single-dish CO profile exhibits emission to±400 km …