Table of Contents
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(I) INTRODUCTION
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Title
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A Giant Molecular Cloud: Orion
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Spectral Energy Distributions of star forming galaxies from UV to radio (M82, Arp 220)
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Correlations between MIR and FIR (IRAS)
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Correlations between MIR and FIR (ISO/IRAS)
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MIR versus Halpha surface brightness in Spiral disks
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UV and extinction: beta-slope
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Comparison of Star Formation Indicators in the Local Universe (Fig.1 of Cram, Mobasher & Rowan-Robinson, 1998)
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Relative Sensitivities to SFR of radio/MIR/sub-mm (template SED of M82 normalized to sensitivity limit for each redshift)
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(II) DEEP SURVEYS
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| MIR (ISOCAM) and sub-mm (SCUBA) deep surveys
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| 15 microns (ISOCAM) integral counts |
(III) NATURE OF ISOCAM GALAXIES
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| Morphologies, colors, masses, L(IR) & SFR of the ISOCAM 15 microns galaxies |
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Chandra X-ray Observatory (CXO) image of HDFN |
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CXO optical identifcations |
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| CXO/ISOCAM identifcations |
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| X-ray luminosities and IR-X power index of ISOCAM/CXO galaxies |
(IV) OPTICAL+NIR KECK SPECTROSCOPY OF ISOCAM GALAXIES
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| Slits on optical galaxies |
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| Comparison SFR Halpha and SFR UV (after correction for extinction from Balmer decremenent, Hbeta/Halpha) |
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| Comparison SFR Halpha (corrected) and SFR MIR |
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| Comparison SFR Halpha(corrected)/SFR Halpha(uncorrected) versus SFR Halpha(uncorrected) |
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| HR10: An Extremely Red Object at z= 1.44 |
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| HR10: A Distant Clone of Arp 220 at z= 1.44 |
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| HR10: model SED |
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| Star formation dependent correction for reddening to reconcile Halpha and FIR in local universe (Hopkins et al. 2001, astro-ph/0103253) |
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| Cosmic IR Background: Origin ? |
(V) MODEL FOR COSMIC IR BACKGROUND AND COSMIC STAR FORMATION HISTORY
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| Number counts in MIR, FIR and Sub-mm: no evolution of the IR luminosity function is ruled out |
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| MIR, FIR, Sub-mm correlations: constraints on template SEDs library |
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| Template SEDs library (Chary & Elbaz 2001) |
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| Luminosity & Density evolution of 15 microns luminosity function: reproduce CIRB |
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| Luminosity & Density evolution of 15 microns luminosity function: reproduce counts, redshift distribution ISOCAM |
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| Cosmic Star Formation History: comparison to other indicators. |
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| Cosmic Star Formation History: when & where did the bulk of present-day stars formed ? |
(VI) CONCLUSIONS
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CONCLUSIONS |
