Other
Scientific paper
Mar 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..381..309c&link_type=abstract
The Second Annual Spitzer Science Center Conference: Infrared Diagnostics of Galaxy Evolution. ASP Conference Series, Vol. 381,
Other
Scientific paper
We present the results of our most recent works on Spitzer/MIPS 24 μ m galaxies. Through a multi-wavelength analysis, we study different properties (redshifts, luminosities, stellar masses) characterizing the sources which produce the bulk of the mid-IR background. From a comparative study with the total population of K_s-selected galaxies, we determine that 24 μ m sources account for an important fraction of the most massive galaxies present at different redshifts. On the other hand, we determine that 24 μ m galaxies also produce most of the energy contained in the far-IR cosmic background at 70 and 160 μ m. Furthermore, we are able to set tight constraints on the Cosmic Infrared Background (CIB) spectral energy distribution (SED). Our results help to clarify the links between these presumably different IR galaxy populations.
Caputi Karina I.
Dole Herve
Lagache Guilaine
Puget Jean-Loop
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