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The XMM deep survey...
The XMM deep survey in the Chandra Deep Field South
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- Comastri, A. (author)
- INAF Osservatorio Astronomico di Bologna
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- Iwasawa, K. (author)
- University of Barcelona,Catalan Institution for Research and Advanced Studies
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- 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
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- Lanzuisi, G. (author)
- INAF Osservatorio Astronomico di Bologna,University of Bologna
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- Gilli, R. (author)
- INAF Osservatorio Astronomico di Bologna
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(creator_code:org_t)
- 2017-03-20
- 2017
- English.
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In: Astronomical Notes - Astronomische Nachrichten. - : Wiley. - 0004-6337. ; 338:2-3, s. 311-315
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Abstract
Subject headings
Close
- 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
Publication and Content Type
- art (subject category)
- ref (subject category)
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