What we learn from the comparison between ISOCAM 15-micron & Spitzer 24-micron source counts

Details What we learn from the comparison between ISOCAM 15-micron & Spitzer 24-micron source counts What we learn from the comparison between ISOCAM 15-micron & Spitzer 24-micron source counts

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005esasp.577..315p&link_type=abstract

In: Proceedings of the dusty and molecular universe: a prelude to Herschel and ALMA, 27-29 October 2004, Paris, France. Ed. by A

Mathematics

Logic

Galaxies: Infrared, Evolution

Scientific paper

The Spitzer Space Telescope is now providing new insights into the IR population contributing to the CIRB, in particular with the MIPS 24-μm band. The question raises on how to compare them with the previous ISOCAM counts at 15-μm. In this work, we present the 24-μm predictions, inferred accurately from a phenomenological 15-μm based model. We will show how extrapolating the ISOCAM populations at higher z, we can explain almost all the 24-μm sources.

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