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

negation

書目名稱Lighthouses of the Universe: The Most Luminous Celestial Objects and Their Use for Cosmology影響因子(影響力)




書目名稱Lighthouses of the Universe: The Most Luminous Celestial Objects and Their Use for Cosmology影響因子(影響力)學(xué)科排名




書目名稱Lighthouses of the Universe: The Most Luminous Celestial Objects and Their Use for Cosmology網(wǎng)絡(luò)公開度




書目名稱Lighthouses of the Universe: The Most Luminous Celestial Objects and Their Use for Cosmology網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Lighthouses of the Universe: The Most Luminous Celestial Objects and Their Use for Cosmology被引頻次




書目名稱Lighthouses of the Universe: The Most Luminous Celestial Objects and Their Use for Cosmology被引頻次學(xué)科排名




書目名稱Lighthouses of the Universe: The Most Luminous Celestial Objects and Their Use for Cosmology年度引用




書目名稱Lighthouses of the Universe: The Most Luminous Celestial Objects and Their Use for Cosmology年度引用學(xué)科排名




書目名稱Lighthouses of the Universe: The Most Luminous Celestial Objects and Their Use for Cosmology讀者反饋




書目名稱Lighthouses of the Universe: The Most Luminous Celestial Objects and Their Use for Cosmology讀者反饋學(xué)科排名

泄露

inquisitive

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?

相一致

Inflammation

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.

傀儡

仔細(xì)檢查

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.

織物

礦石

出汗

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.