At low redshift, only about one-tenth of the known baryons lie in galaxies or the hot gas seen
in galaxy clusters and groups. Models posit that these “missing baryons” are in gaseous …

Aims. We study the relationship between the local environment of galaxies and their star
formation rate (SFR) in the Great Observatories Origins Deep Survey, GOODS, at. Methods …

Template fits to observed galaxy fluxes allow calculation of K-corrections and conversions
among observations of galaxies at various wavelengths. We present a method for creating …

The DEEP2 and COMBO-17 surveys are compared to study luminosity functions of red and
blue galaxies to z~ 1. The two surveys have different methods and sensitivities, but …

With the goal of investigating the degree to which the MIR emission traces the SFR, we
analyze Spitzer 8 and 24 μm data of star-forming regions in a sample of 33 nearby galaxies …

We present images, integrated photometry, and surface-brightness and color profiles for a
total of 1034 nearby galaxies recently observed by the Galaxy Evolution Explorer (GALEX) …

We have analyzed the bivariate distribution of galaxies as a function of ultraviolet-optical
colors and absolute magnitudes in the local universe. The sample consists of galaxies with …

Abstract We use the Sloan Digital Sky Survey (SDSS) to construct a sample of 625 brightest
group and cluster galaxies (BCGs) together with control samples of non-BCGs matched in …

We use a sample of 43,690 galaxies selected from the Sloan Digital Sky Survey Data
Release 4 to study the systematic effects of specific star formation rate (SSFR) and galaxy …

We introduce a new quantity, the mass flux density of galaxies evolving from the blue
sequence to the red sequence. We propose a simple technique for constraining this mass …