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

Pozzi, Francesca, Gruppioni, C, Lari, C, Oliver, S and Rodighiero, G. (2005) What we learn from the comparison between ISOCAM 15-micron & Spitzer 24-micron source counts. In: Proceedings of the dusty and molecular universe: a prelude to Herschel and ALMA, 27-29 October 2004, 27-29 October 2004., Paris, France.

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Abstract

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.

Item Type: Conference or Workshop Item (Paper)
Additional Information: Published in: Proceedings of the dusty and molecular universe: a prelude to Herschel and ALMA, 27-29 October 2004, Paris, France. Ed. by A. Wilson. ESA SP-577, Noordwijk, Netherlands: ESA Publications Division, ISBN 92-9092-855-7, 2005, p. 315 - 316
Schools and Departments: School of Mathematical and Physical Sciences > Physics and Astronomy
Depositing User: Seb Oliver
Date Deposited: 06 Feb 2012 20:17
Last Modified: 30 Nov 2012 17:06
URI: http://srodev.sussex.ac.uk/id/eprint/25146
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