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

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.
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].
File in questo prodotto:
File Dimensione Formato  
aa4904-06.pdf

accesso aperto

Dimensione 1.78 MB
Formato Adobe PDF
1.78 MB Adobe PDF Visualizza/Apri

I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/10447/30665
Citazioni
  • ???jsp.display-item.citation.pmc??? ND
  • Scopus 56
  • ???jsp.display-item.citation.isi??? 60
social impact