The XMM-Newton survey of the ELAIS-S1 field I. Number counts, angular correlation function and X-ray spectral properties

Astronomy and Astrophysics

Volumn 457, Issue 2, 2006, Pages 501-515

  Puccetti, S ^a,b   Flore, F ^a   D'Elia, V ^a   Pillitteri, I ^c   Feruglio, C ^a   Grazian, A ^a   Brusa, M ^d   Ciliegi, P ^e   Comastri, A ^e   Gruppioni, C ^e   Mignoli, M ^e   Vignali, C ^f   Zamorani, G ^e   La Franca, F ^g   Sacchi, N ^g   Franceschini, A ^h   Berta, S ^h   Buttery, H ⁱ   Dias, J E ⁱ  

^a INAF OSSERVATORIO ASTRONOMICO DI ROMA   (Italy)

^b UNIVERSITY OF ROME TOR VERGATA   (Italy)

^c UNIVERSITY OF PALERMO   (Italy)

^d MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^e OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

^f UNIVERSITY OF BOLOGNA   (Italy)

^g ROMA TRE UNIVERSITY   (Italy)

^h UNIVERSITY OF PADOVA   (Italy)

ⁱ INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

Author keywords

Galaxies: active; Large scale structure of Universe; X rays: galaxies

Indexed keywords

ANGULAR CORRELATION FUNCTION; GALAXIES: ACTIVE; LARGE-SCALE STRUCTURE OF UNIVERSE; X-RAYS: GALAXIES;

GALAXIES; GAS EMISSIONS; MATHEMATICAL MODELS; OPTICAL CORRELATION; SPECTRUM ANALYSIS; X RAYS;

ASTROPHYSICS;

EID: 33749586184     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20064904     Document Type: Article

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