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X-rays from the first massive black holes
Authors:WN Brandt  C Vignali  DP Schneider  DM Alexander  SF Anderson  FE Bauer  X Fan  GP Garmire  S Kaspi  GT Richards  
Institution:

a525 Davey Laboratory, Department of Astronomy and Astrophysics, The Pennsylvania State University, University Park, PA 16802, USA

bDepartment of Astronomy, University of Washington, P.O. Box 351580, Seattle, WA 98195, USA

cSteward Observatory, The University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, USA

dThe Raymond and Beverly Sackler Faculty of Exact Sciences, School of Physics and Astronomy and the Wise Observatory, Tel-Aviv University, Tel-Aviv 69978, Israel

ePrinceton University Observatory, Princeton, NJ 08544, USA

Abstract:X-ray studies of high-redshift (z > 4) active galaxies have advanced substantially over the past few years, largely due to results from the new generation of X-ray observatories. As of this writing X-ray emission has been detected from nearly 60 high-redshift active galaxies. This paper reviews the observational results and their implications for models of the first massive black holes, and it discusses future prospects for the field.
Keywords:Massive black holes  X-ray astronomy  High-redshift active galaxies
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