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.
| Lingua originale | English |
|---|---|
| pagine (da-a) | 501-515 |
| Numero di pagine | 15 |
| Rivista | ASTRONOMY & ASTROPHYSICS |
| Volume | 457 |
| Stato di pubblicazione | Published - 2006 |
| Pubblicato esternamente | Yes |
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Cita questo
Pillitteri, I. F., & Delia, V. (2006). The XMM-Newton survey of the ELAIS-S1 field. I. Number counts, angular correlation function and X-ray spectral properties. ASTRONOMY & ASTROPHYSICS, 457, 501-515.