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A&A 453, L5-L8 (2006)
DOI: 10.1051/0004-6361:20065157
Letter
Coma revealed as an extended hard X-rays source by INTEGRAL IBIS/ISGRI
M. Renaud1, 2, G. Bélanger1, 2, J. Paul1, 2, F. Lebrun1, 2 and R. Terrier21 Service d'Astrophysique, CEA-Saclay, 91191 Gif-Sur-Yvette, France
e-mail: mrenaud@cea.fr
2 APC-UMR 7164, 11 place M. Berthelot, 75231 Paris, France
(Received 7 March 2006 / Accepted 26 April 2006)
Abstract
Aims.We report the INTEGRAL/IBISobservations of the Coma Clusterin the hard
X-ray/soft
-raydomain.
Methods.Since the Coma Clusterappears as an extended source,
its global intensity and significance cannot be directly extracted with standard
coded mask analysis. We used the method of imaging the extended sources with
a coded mask telescope developed by Renaud et al. (2006).
Results.The imaging capabilities
and the sensitivity of the IBIS/ISGRIcoded mask instrument allows us to identify
for the first time the site of the emission above ~15 keV. We have studied
the Coma Clustermorphology in the 18-30 keV band and found that it follows the
prediction based on X-rayobservations. We also bring constraints on the non-thermal
mechanism contribution at higher energies.
Key words: galaxies: clusters: Coma Cluster -- methods: data analysis -- gamma rays: observations -- X-rays: galaxies: clusters
© ESO 2006
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