Herschel/hermes: Bivariate UV/IR Luminosity Functions At Z 1.5

Details Herschel/hermes: Bivariate UV/IR Luminosity Functions At Z 1.5 Herschel/hermes: Bivariate UV/IR Luminosity Functions At Z 1.5

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aas...21922906h&link_type=abstract

American Astronomical Society, AAS Meeting #219, #229.06

Astronomy and Astrophysics

Astronomy

Scientific paper

We study the infrared properties of a sample of ultraviolet (UV) selected galaxies at z 1.5. Using stacking at 250um, 350um and 500 um from the SPIRE imaging of the COSMOS field obtained within the HerMES key program, we derive the mean total infrared luminosity as a function of UV luminosity and slope of the UV continuum. The infrared to UV luminosity ratio does not depend on UV luminosity in the range 5×109

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