The high-redshift (z > 3) active galactic nucleus population in the 4-Ms Chandra Deep Field-South

Monthly Notices of the Royal Astronomical Society

Volumn 428, Issue 1, 2013, Pages 354-369

  Vito, F ^a,b   Vignali, C ^a,b   Gilli, R ^b   Comastri, A ^b   Iwasawa, K ^c   Brandt, W N ^d   Alexander, D M ^e   Brusa, M ^f   Lehmer, B ^g,h   Bauer, F E ^i,j   Schneider, D P ^d   Xue, Y Q ^k   Luo, B ^d  

^a UNIVERSITY OF BOLOGNA   (Italy)

^b OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

^c UNIVERSITY OF BARCELONA   (Spain)

^d PENNSYLVANIA STATE UNIVERSITY   (United States)

^e DURHAM UNIVERSITY   (United Kingdom)

^f MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^g JOHNS HOPKINS UNIVERSITY   (United States)

^h NASA GODDARD SPACE FLIGHT CENTER   (United States)

ⁱ PONTIFICIA UNIVERSIDAD CATÓLICA DE CHILE   (Chile)

^j Center for Extrasolar Planetary Systems   (United States)

^k UNIVERSITY OF SCIENCE AND TECHNOLOGY OF CHINA   (China)

more..

Author keywords

Aactive galaxies; Data analysis techniques; Galaxies; High redshift X rays; Imaging spectroscopy surveys galaxies; Methods

Indexed keywords

EID: 84872393221     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1093/mnras/sts034     Document Type: Article

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