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  1. OA@INAF
  2. PRODOTTI RICERCA INAF
  3. 1 CONTRIBUTI IN RIVISTE (Journal articles)
  4. 1.01 Articoli in rivista
Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12386/28424
Title: X-Ray Properties of AGN in Brightest Cluster Galaxies. I. A Systematic Study of the Chandra Archive in the 0.2 < z < 0.3 and 0.55 < z < 0.75 Redshift Range
Authors: YANG, LILAN
TOZZI, Paolo 
Yu, Heng
LUSSO, ELISABETA
GASPARI, MASSIMO 
GILLI, Roberto 
NARDINI, EMANUELE 
RISALITI, Guido
Issue Date: 2018
Journal: THE ASTROPHYSICAL JOURNAL 
Number: 859
Issue: 1
First Page: 65
Abstract: We present a search for nuclear X-ray emission in the brightest cluster galaxies (BCGs) of a sample of groups and clusters of galaxies extracted from the Chandra archive. The exquisite angular resolution of Chandra allows us to obtain robust photometry at the position of the BCG, and to firmly identify unresolved X-ray emission when present, thanks to an accurate characterization of the extended emission at the BCG position. We consider two redshift bins (0.2 < z < 0.3 and 0.55 < z < 0.75) and analyze all the clusters observed by Chandra with exposure time larger than 20 ks. Our samples have 81 BCGs in 73 clusters and 51 BCGs in 49 clusters in the low- and high-redshift bins, respectively. X-ray emission in the soft (0.5-2 keV) or hard (2-7 keV) band is detected only in 14 and 9 BCGs (∼18% of the total samples), respectively. The X-ray photometry shows that at least half of the BCGs have a high hardness ratio, compatible with significant intrinsic absorption. This is confirmed by the spectral analysis with a power-law model plus intrinsic absorption. We compute the fraction of X-ray bright BCGs above a given hard X-ray luminosity, considering only sources with positive photometry in the hard band (12/5 sources in the low/high-z sample).
URI: http://hdl.handle.net/20.500.12386/28424
URL: https://arxiv.org/abs/1804.08633
https://iopscience.iop.org/article/10.3847/1538-4357/aabfd7
ISSN: 0004-637X
DOI: 10.3847/1538-4357/aabfd7
Bibcode ADS: 2018ApJ...859...65Y
Fulltext: open
Appears in Collections:1.01 Articoli in rivista

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