A Far-ir Characterization Of 24 Micron Selected Galaxies At 0 < Z < 2.5 Using Stacking At 70 Microns And 160 Microns In The Cosmos Field

Details A Far-ir Characterization Of 24 Micron Selected Galaxies At 0 < Z < 2.5 Using Stacking At 70 Microns And 160 Microns In The Cosmos Field A Far-ir Characterization Of 24 Micron Selected Galaxies At 0 < Z < 2.5 Using Stacking At 70 Microns And 160 Microns In The Cosmos Field

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21733538l&link_type=abstract

American Astronomical Society, AAS Meeting #217, #335.38; Bulletin of the American Astronomical Society, Vol. 43, 2011

Astronomy and Astrophysics

Astronomy

Scientific paper

We present a study of the average properties of luminous infrared galaxies detected directly at 24 µm in the COSMOS field using a median stacking analysis at 70 µm and 160 µm. Over 35000 sources spanning 0

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