Image Details
Caption: Fig. 2.
Hardness ratios HR = (H − S)/(H + S) (left ordinate axis) of X‐ray sources vs. their full‐band (0.5–10.0 keV) X‐ray fluxes. The photon indices Γ of the power‐law spectra that could reproduce the observed hardness ratios are given along the right ordinate (see text for details). The dotted line connects the averaged hardness ratios for detected sources within different flux bins.
© 2004. The American Astronomical Society. All rights reserved. Printed in U.S.A.