arXiv · astro-ph/0312625
Confirmation of non-thermal hard X-ray excess in the Coma cluster from two epoch observations
Abstract
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.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Roberto Fusco-Femiano, Mauro Orlandini, Gianfranco Brunetti, Luigina Feretti, Gabriele Giovannini, Paola Grandi, Giancarlo Setti. 2003-12-26. Confirmation of non-thermal hard X-ray excess in the Coma cluster from two epoch observations. https://doi.org/10.1086/382695
Cite the original work for its findings. Save a collection to share your selection of sources.