Titlebook: Lighthouses of the Universe: The Most Luminous Celestial Objects and Their Use for Cosmology; Proceedings of the M Marat Gilfanov,Rashid Su

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Resolving the Cosmic Infrared Background with ISOCAM,e also harbor an AGN. In the local universe, LIGs and ULIGs together emit less than 10% of the IR light, and less than 2% of the bolometric light. Is their contribution much more important at large distances? Are they ultimately responsible for the CIRB?

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Far-Infrared and Submillimetre Lighthouses,ar populations has already been formed. It is a challenge to account for such a large population of high-redshift luminous galaxies. The relation of these observations to the problem of accounting for the evolution of the cosmic star formation rate is discussed.

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Conference proceedings 2002robes of the intergalactic medium at high redshifts and as a tool to study the end of dark ages. The theoretical models are complemented by new exciting results from orbital and ground-based observatories such as Chandra, XMM-Newton, HST, SDSS, VLT, Keck, and many others.

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First Results from the ESO Distant Cluster Survey,btain measurements of the masses of the clusters. We also perform a bulge-disk decomposition on the cluster galaxies, and find that, with two notable exceptions, the higher mass clusters have a higher fraction of bulge dominated galaxies.