X-rays from the First Massive Black Holes

Simple item page
dc.creatorBrandt, W. N.
dc.creatorVignali, C.
dc.creatorSchneider, D. P.
dc.creatorAlexander, D. M.
dc.creatorAnderson, S. F.
dc.creatorBauer, F. E.
dc.creatorFan, X.
dc.creatorGarmire, G. P.
dc.creatorKaspi, S.
dc.creatorRichards, G. T.
dc.date2002-12-03
dc.date2003-02-05
dc.date.accessioned2026-07-07T02:06:41Z
dc.date.available2026-07-07T02:06:41Z
dc.descriptionX-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.
dc.description10 pages; in New X-ray Results from Clusters of Galaxies and Black Holes (Oct 2002; Houston, TX), eds. C. Done, E.M. Puchnarewicz, M.J. Ward, Advances in Space Research; list of z > 4 X-ray detections available from http://www.astro.psu.edu/users/niel/papers/papers.html
dc.identifierhttps://arxiv.org/abs/astro-ph/0212082
dc.identifierhttp://arxiv.org/abs/astro-ph/0212082
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5451
dc.subjectAstrophysics
dc.titleX-rays from the First Massive Black Holes
dc.typetext

Files

Collections

arXiv