The cross-correlation of faint QSOs with the cosmic X-ray background

Por: Miyaji T., Ogasaka Y., Boldt E., Connolly A.J., Szalay A.S., Koo D.C., Kii T., Inoue H., Kunieda H., Tawara Y.

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Publicada: 1 ene 1998

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Filiaciones:
Miyaji T.:
 Astrophysikalisches Institut Potsdam, An der Sternwarte 16, D-14482 Potsdam, Germany

Ogasaka Y.:
 LHEA, NASA Goddard Space Flight Center, Greenbelt, MD 20771, United States

Boldt E.:
 LHEA, NASA Goddard Space Flight Center, Greenbelt, MD 20771, United States

Connolly A.J.:
 Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD 21218, United States

Szalay A.S.:
 Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD 21218, United States

Koo D.C.:
 UCO/Lick Observatory, University of California, Santa Cruz, CA 95064, United States

Kii T.:
 ISAS, 3-1-1 Yoshinodai, Sagamihara, Kanagawa, 229, Japan

Inoue H.:
 ISAS, 3-1-1 Yoshinodai, Sagamihara, Kanagawa, 229, Japan

Kunieda H.:
 Department of Astrophysics, Nagoya University, Nagoya, 464-01, Japan

Tawara Y.:
 Department of Astrophysics, Nagoya University, Nagoya, 464-01, Japan