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Confirmation of Nonthermal Hard X-Ray Excess in the Coma Cluster from Two Epoch Observations
Author(s) -
R. FuscoFemiano,
M. Orlandini,
G. Brunetti,
L. Feretti,
G. Giovannini,
P. Grandi,
Giancarlo Setti
Publication year - 2004
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/382695
Subject(s) - coma cluster , astrophysics , physics , coma (optics) , spectral line , flux (metallurgy) , sigma , cluster (spacecraft) , epoch (astronomy) , astronomy , galaxy cluster , galaxy , materials science , computer science , metallurgy , programming language
We report the hard X-ray spectrum of the Coma cluster obtained using the PDS data of two independent BeppoSAX observations performed with a time interval of about three years. In both the spectra a non thermal excess with respect to the thermal emission is present at a confidence level of ~ 3.4 sigma. The combined spectrum obtained by adding up the two spectra allows a measurement of the excess at the level of ~ 4.8 sigma at energies above 20 keV. The analysis of the full BeppoSAX data set provides a revised non-thermal X-ray flux which is slightly lower than that previously estimated (Fusco-Femiano et al. 1999) and in agreement with that measured by two RXTE observations. The analysis of the offset fields in our Coma observations provides a possible flux determination of the BL Lac object 1ES 1255+244

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