Aims. The formation and evolution of cosmic structures can be probed by studying the evolution of the luminosity function of the Active Galactic Nuclei (AGNs), galaxies and clusters of galaxies and of the clustering of the X-ray active Universe, compared to the IR-UV active Universe.
S PUCCETTI, F FIORE, V D'ELIA, PILLITTERI I, C FERUGLIO, A GRAZIAN, et al. (2006). The XMM-Newton survey of the ELAIS-S1 field. I. Number counts, angular correlation function and X-ray spectral properties. ASTRONOMY & ASTROPHYSICS, 457(2), 501-515 [10.1051/0004-6361:20064904].
The XMM-Newton survey of the ELAIS-S1 field. I. Number counts, angular correlation function and X-ray spectral properties
DELIA, Vincenzo;PILLITTERI, Ignazio Francesco;
2006-01-01
Abstract
Aims. The formation and evolution of cosmic structures can be probed by studying the evolution of the luminosity function of the Active Galactic Nuclei (AGNs), galaxies and clusters of galaxies and of the clustering of the X-ray active Universe, compared to the IR-UV active Universe.
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