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تسجيل مستخدم جديدThe spectrum of the cosmic X-ray background observed by RTXE/PCA
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We have analyzed a large set of RXTE/PCA scanning and slewing observations performed between April 1996 and March 1999. We obtained the 3-20 keV spectrum of the cosmic X-ray background (CXB) by subtracting Earth-occulted observations from observations of the X-ray sky at high galactic latitude and far away from sources. The sky coverage is approximately ~22600 sq.deg. The PCA spectrum of CXB in 3-20 keV energy band is adequately approximated by a single power law with photon index Gamma~1.4 and normalization at 1 keV ~9.5 phot/s/cm2/keV/sr. Instrumental background uncertainty precludes accurate RXTE/PCA measurements of the spectrum of cosmic X-ray background at energies above 15 keV and therefore we can not detect the high energy cutoff observed by HEAO-1 A2 experiment. Deep observations of the 6 high latitude points used to model the PCA background provide a coarse measure of the spatial variation of the CXB. The CXB variations are consistent with a fixed spectral shape and variable normalization characterized by a fractional rms amplitude of ~7% on angular scales of ~1 square deg.
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