The X-ray spectral properties of the AGN population in the XMM-Newton bright serendipitous survey

Astronomy and Astrophysics

Volumn 530, Issue , 2011, Pages

  Corral, A ^a   Della Ceca, R ^a   Caccianiga, A ^a   Severgnini, P ^a   Brunner, H ^b   Carrera, F J ^c   Page, M J ^d   Schwope, A D ^e  

^a INAF IASF MILANO   (Italy)

^b MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^c INSTITUTO DE FÍSICA DE CANTABRIA CSIC UC   (Spain)

^d UNIVERSITY COLLEGE LONDON   (United Kingdom)

^e ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

Author keywords

Galaxies: active; Surveys; X rays: diffuse background; X rays: general

Indexed keywords

ACTIVE GALACTIC NUCLEI; COLUMN DENSITY; CONFIDENCE LEVELS; DIFFERENT ORIGINS; EMISSION LINES; ENERGY BAND; EQUIVALENT WIDTH; GALAXIES : ACTIVE; HARD X RAY; HIGH-REDSHIFT; INTRINSIC ABSORPTIONS; LINE EMISSIONS; MASSIVE BLACK HOLES; PHOTON INDEX; POWER-LAW; RED SHIFT; SPECTRAL ANALYSIS; SPECTRAL INDICES; SPECTRAL PROPERTIES; UPPER LIMITS; X RAY SPECTRUM; X-RAY SPECTRA; X-RAY SURVEYS; X-RAYS: DIFFUSE BACKGROUND; X-RAYS: GENERAL; XMM-NEWTON;

GALAXIES; LUMINANCE; SPECTRUM ANALYSIS; SURVEYS; X RAY SPECTROGRAPHS; X RAYS;

X RAY ANALYSIS;

EID: 79955640336     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201015227     Document Type: Article

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