The XMM Deep Survey in the CDF-S

2014/11/28 by M. Antonucci, A. Talavera, F. Vagnetti +6
Physics and Astronomy · #Active galactic nucleus #Astrophysical Phenomena and Observations #Astrophysics #Astrophysics and Cosmic Phenomena #Chandra Deep Field South #Environmental science #Galaxies: Formation, Evolution, Phenomena #Galaxy #Geology #Observatory #Physics #Remote sensing #astro-ph.CO #astro-ph.GA

paper · pdf · doi:10.1051/0004-6361/201425010

published as A&A 574, A49 (2015) · Change of numbering in the title, language corrections, version corresponding to that in press, 15 pages, 12 Figures, to appear on Astronomy and Astrophysics. Data available at https://www.fisica.uniroma2.it/~tovastro/ea/xmmomcdfs.html

openalex publication_date 2014/11/28 · arxiv created 2014/12/01 · arxiv updated 2015/01/28 · openalex created_date 2020/11/23 · openalex updated_date 2026/08/05

Abstract

Context. The XMM-Newton X-ray observatory has repeatedly observed the Chandra Deep Field-South (CDF-S) in 33 epochs (2001–2010) through the XMM-CDFS Deep Survey. During the X-ray observations, XMM-OM targeted the central 17 × 17 arcmin2 region of the X-ray field of view, providing simultaneous optical/UV coverage of the CDF-S. The resulting set of data can be used to build an XMM-OM catalogue of the CDF-S, filling the UV spectral coverage between the optical surveys and GALEX observations.

Citations

• The Blast Wave Model for AGN Feedback: Effects on AGN Obscuration
• The synthesis of the cosmic X-ray background in the Chandra and XMM-Newton era
• The Evolutionary Sequence of Active Galactic Nuclei and Galaxy Formation Revealed
• Calibration update of the COMBO-17 CDFS catalogue
• Are Optically Selected Quasars Universally X‐Ray Luminous? X‐Ray–UV Relations in Sloan Digital Sky Survey Quasars
• Prevalence of X‐Ray Variability in the Chandra Deep Field–South
• The Hubble Ultra Deep Field
• Variability and the X-ray/UV ratio of active galactic nuclei
• The Chandra Deep Field–South: Optical Spectroscopy. I.
• The USNO-B Catalog
• The Great Observatories Origins Deep Survey

Cited by

• The XMM deep survey in the CDF-S II. a 9-20 keV selection of heavily obscured active galaxies at z>1.7