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A survey of hard spectrum ROSAT sources 1: X-ray source catalogue | | M.J. Page
; J.P.D. Mittaz
; F.J. Carrera
; | | Date: |
24 Jun 2000 | | Journal: | Mon.Not.Roy.Astron.Soc. 318 (2000) 1073 | | Subject: | astro-ph | | Affiliation: | MSSL), J.P.D. Mittaz (MSSL), F.J. Carrera (MSSL, Ifca | | Abstract: | We present a catalogue of 147 serendipitous X-ray sources selected to have hard spectra (alpha < 0.5) from a survey of 188 ROSAT fields. Such sources must be the dominant contributors to the X-ray background at faint fluxes. We have used Monte Carlo simulations to verify that our technique is very efficient at selecting hard sources: the survey has > 10 times as much effective area to hard sources as it has to soft sources above a 0.5 - 2 keV flux level of 10^-14 erg/cm^2/s. The distribution of best fit spectral slopes of the hard sources suggests that a typical ROSAT hard source in our survey has a spectral slope alpha ~0. The hard sources have a steep number flux relation (dN/dS propto S^-gamma with a best fit value of gamma = 2.72 +- 0.12) and make up about 15% of all 0.5 - 2 keV sources with S > 10^-14 erg/cm^2/s. If their N(S) continues to fainter fluxes, the hard sources will comprise ~ 40% of sources with 5 10^-15 < S < 10^-14. The population of hard sources can therefore account for the harder average spectra of ROSAT sources with S < 10^-14. They probably make a strong contribution to the X-ray background at faint fluxes and could be the solution to the X-ray background spectral paradox. | | Source: | arXiv, astro-ph/0006347 | | Services: | Forum | Review | PDF | Favorites | |
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