Abstract
The origin of the X-ray background, in particular at hard (2-10 keV) energies, is an issue that has been debated for more than 40 years. The Chandra Deep Fields provide the deepest look at the X-ray sky and are the best data set to study the X-ray background. We searched the Chandra Deep Field-South for X-ray sources with the aid of a dedicated wavelet-based algorithm. We are able to reconstruct the log N-log S source distribution in the soft (0.5-2 keV) and hard (2-10 keV) bands down to limiting fluxes of 2 × 10-17 and 2 × 10-16 ergs s-1 cm-2, respectively. These are a factor of ~5 deeper than previous investigations. We find that the soft relation continues along the extrapolation from higher fluxes, almost completely accounting for the soft X-ray background. On the contrary, the hard distribution shows a flattening below ~2 × 10-14 ergs s-1 cm-2. Nevertheless, we can account for 68% of the hard X-ray background, with the main uncertainty being the sky flux itself.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
