C. Gruppioni, F. Pozzi, C. Lari, S. Oliver, G. Rodighiero
Published 2004-11-16, updated 2004-11-26Version 2
The comparison between the new Spitzer data at 24 micron and the previous ISOCAM data at 15 micron is a key tool to understand galaxy properties and evolution in the infrared and to interpret the observed number counts, since the combination of Spitzer with the ISO cosmological surveys provides for the first time the direct view of the Universe in the Infrared up to z~2. We present the prediction in the Spitzer 24-micron band of a phenomenological model for galaxy evolution derived from the 15-micron data. Without any ``a posteriori'' update, the model predictions seem to agree well with the recently published 24-micron extragalactic source counts, suggesting that the peak in the 24-micron counts is dominated by ``starburst'' galaxies like those detected by ISOCAM at 15 micron, but at higher redshifts (1 < z < 2 instead of 0.5 < z < 1.5).
Comments: 8 pages: 4 pages of main text + 5 postscript figures, use aastex. Accepted for publication in ApJL. Replaced with the proof version (added missing references and corrected a few sentences)
Journal: Astrophys.J. 618 (2004) L9-L12
The SCUBA 8-mJy survey - I: Sub-millimetre maps, sources and number counts
Effect of clustering on extragalactic source counts with low-resolution instruments
Extragalactic Source Counts at 24 Microns in the Spitzer First Look Survey
