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The XMM deep survey in the Chandra Deep Field South

Comastri, A. (author)
INAF Osservatorio Astronomico di Bologna
Iwasawa, K. (author)
University of Barcelona,Catalan Institution for Research and Advanced Studies
Centis Vignali, M (author)
INAF Osservatorio Astronomico di Bologna
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Ranalli, P. (author)
Lund University,Lunds universitet,Astronomi - Genomgår omorganisation,Institutionen för astronomi och teoretisk fysik - Genomgår omorganisation,Naturvetenskapliga fakulteten,Lund Observatory - Undergoing reorganization,Department of Astronomy and Theoretical Physics - Undergoing reorganization,Faculty of Science
Lanzuisi, G. (author)
INAF Osservatorio Astronomico di Bologna,University of Bologna
Gilli, R. (author)
INAF Osservatorio Astronomico di Bologna
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 (creator_code:org_t)
2017-03-20
2017
English.
In: Astronomical Notes - Astronomische Nachrichten. - : Wiley. - 0004-6337. ; 338:2-3, s. 311-315
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • The Chandra Deep Field South (CDF-S) was observed by XMM-Newton for about 3Ms in many periods over the past decade (2001-2002 and 2008-2009). The main goal of the survey was to obtain good quality X-ray spectroscopy of the active galactic nuclei responsible for the bulk of the X-ray background. We present the scientific highlights of the XMM-Newton survey and briefly discuss the perspectives of future observations to pursue XMM deep survey science with current and forthcoming X-ray facilities.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

Galaxies: active
X-rays: galaxies

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Comastri, A.
Iwasawa, K.
Centis Vignali, ...
Ranalli, P.
Lanzuisi, G.
Gilli, R.
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NATURAL SCIENCES
NATURAL SCIENCES
and Physical Science ...
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Lund University

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