High precision X-ray log N - Log S distributions: Implications for the obscured AGN population

被引：0

作者：

Mateos, S. ^{[1
]}

Warwick, R.S. ^{[1
]}

Carrera, F.J. ^{[2
]}

Stewart, G.C. ^{[1
]}

Ebrero, J. ^{[1
,2
]}

Della Ceca, R. ^{[3
]}

Caccianiga, A. ^{[3
]}

Gilli, R. ^{[4
]}

Page, M.J. ^{[5
]}

Treister, E. ^{[6
]}

Tedds, J.A. ^{[1
]}

Watson, M.G. ^{[1
]}

Lamer, G. ^{[7
]}

Saxton, R.D. ^{[8
]}

Brunner, H. ^{[9
]}

Page, C.G. ^{[1
]}

机构：

[1] X-ray Astronomy Group, Department of Physics and Astronomy, Leicester University, Leicester LE1 7RH, United Kingdom

[2] Instituto de Física de Cantabria (CSIC-UC), 39005 Santander, Spain

[3] INAF, Osservatorio Astronomico di Brera, via Brera 28, 20121 Milan, Italy

[4] Istituto Nazionale di Astrofisica (INAF), Osservatorio Astronomico di Bologna, via Ranzani 1, 40127 Bologna, Italy

[5] Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey RH5 6NT, United Kingdom

[6] European Southern Observatory, Casilla 19001, Santiago 19, Chile

[7] Astrophysikalisches Institut Potsdam, An der Sternwarte 16, 144482 Potsdam, Germany

[8] XMM SOC, ESAC, Apartado 78, 28691 Villanueva de la Caada, Madrid, Spain

[9] Max-Planck-Institut für Extraterrestrische Physik, Giessenbachstrasse, Garching 85748, Germany

来源：

Astronomy and Astrophysics | 2008年 / 492卷 / 01期

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摘要：

Journal article (JA)

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页码：51 / 69