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Resolving the 10-40 keV Cosmic X-ray Background with Constellation-X | | Giorgio Matt
; Fulvio Pompilio
; Fabio La Franca
; | | Date: |
8 Jul 2000 | | Subject: | astro-ph | | Affiliation: | Dip. Fisica, Univ. Roma Tre | | Abstract: | The energy density of the Cosmic X-ray background (XRB) peaks around 30 keV (see Figure 1), an energy not yet probed by focussing imaging instruments. The first hard X-ray telescope due to fly on a space mission will be that on board Constellation-X. The imaging capability, besides providing an improvement of several orders of magnitude in sensitivity over current passively collimated detectors, will permit for the first time to resolve a fraction of the XRB at this most crucial energy. Synthesis models of the XRB based on obscured AGN predict that at least 40% of the 10-40 keV XRB will be resolved by Constellation-X. | | Source: | arXiv, astro-ph/0007106 | | Services: | Forum | Review | PDF | Favorites | |
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