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A New Technique for Determining the Number of X-Ray Sources per Flux Density Interval

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© 2003. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation A. T. Kenter and S. S. Murray 2003 ApJ 584 1016 DOI 10.1086/345790

0004-637X/584/2/1016

Abstract

We present a technique for determining the number of X-ray sources per flux density interval, the log N-log S relationship, that is mathematically analogous to spectral fitting. This technique is ideal for X-ray source counts obtained using the Chandra X-ray Observatory since the telescope and the focal plane instruments have been well modeled. This technique is of general applicability. In this paper, we apply it to a wavelet source-detect analysis of a Chandra Advanced CCD Imaging Spectrometer (ACIS-I) mosaic image of a 1.35 deg2 survey of the Lockman Hole. We verify the technique via Monte Carlo simulations.

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10.1086/345790