Image Details
Caption: Fig. 3.
Observed energy dependence of the burst oscillation amplitudes (MOC03, triangles with error bars), in comparison with our full numerical calculations using ﹩k_{\mathrm{B}\,}T_{c}=3﹩ keV (solid lines). We label each panel with the NS name and the epoch of the measurements if that NS was observed over multiple epochs. For each calculation the spin is set to that object’s burst oscillation frequency, and the normalization is set to maximize the fit.
© 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A.