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Enhanced Dense Gas Fraction in Ultra-Luminous Infrared Galaxies
S. Juneau, D. T. Narayanan, J. Moustakas +4
We present a detailed analysis of the relation between infrared luminosity and molecular line luminosity, for a variety of molecular transitions, using a sample of 34 nearby galaxi…
A Spectroscopically Confirmed Excess of 24 micron Sources in a Super Galaxy Group at z=0.37: Enhanced Dusty Star Formation Relative to the Cluster and Field Environment
Kim-Vy H. Tran, Amelie Saintonge, John Moustakas +5
To trace how dust-obscured star formation varies with environment, we compare the fraction of 24 micron sources in a super galaxy group to the field and a rich galaxy cluster at z~…
Radial distribution of stars, gas and dust in SINGS galaxies. II. Derived dust properties
J. C. Muñoz-Mateos, A. Gil de Paz, S. Boissier +13
We present a detailed analysis of the radial distribution of dust properties in the SINGS sample, performed on a set of UV, IR and HI surface brightness profiles, combined with pub…
Radial distribution of stars, gas and dust in SINGS galaxies. I. Surface photometry and morphology
J. C. Muñoz-Mateos, A. Gil de Paz, J. Zamorano +11
We present ultraviolet through far-infrared surface brightness profiles for the 75 galaxies in the Spitzer Infrared Nearby Galaxies Survey (SINGS). The imagery used to measure the…
Low Resolution Spectral Templates For AGNs and Galaxies From 0.03 -- 30 microns
R. J. Assef, C. S. Kochanek, M. Brodwin +9
We present a set of low resolution empirical SED templates for AGNs and galaxies in the wavelength range from 0.03 to 30 microns based on the multi-wavelength photometric observati…
Physical properties and environments of nearby galaxies
Michael R. Blanton, John Moustakas
We review the physical properties of nearby, relatively luminous galaxies, using results from newly available massive data sets together with more detailed observations. First, we…