Exploring the X-ray sky with the XMM-Newton bright serendipitous survey

Astronomy and Astrophysics

Volumn 428, Issue 2, 2004, Pages 383-399

  Della Ceca, R ^a   Maccacaro, T ^a   Caccianiga, A ^a   Severgnini, P ^a   Braito, V ^a   Barcons, X ^b   Carrera, F J ^b   Watson, M G ^c   Tedds, J A ^c   Brunner, H ^d   Lehmann, I ^d   Page, M J ^e   Lamer, G ^f   Schwope, A ^f  

^a INAF IASF MILANO   (Italy)

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

^c UNIVERSITY OF LEICESTER   (United Kingdom)

^d MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^e UNIVERSITY COLLEGE LONDON   (United Kingdom)

^f ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

Author keywords

Surveys; X rays: active galaxies; X rays: diffuse background

Indexed keywords

BAND STRUCTURE; CAMERAS; DATA REDUCTION; PARAMETER ESTIMATION; PROBABILITY; SPECTROSCOPY; SPECTRUM ANALYSIS; SURVEYS;

DIFFUSE BACKGROUND; HARD BRIGHT SOURCE SAMPLE (HBSS); NEWTON FIELDS; X RAYS:ACTIVE GALAXIES;

X RAY ANALYSIS;

EID: 10844232897     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20040252     Document Type: Review

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