Fig. 4
Spectral modeling of the joint data. Top: unfolded XMM-Newton, RXTE and INTEGRAL data and best fit model components for the Corona geometry for Obs2. Blue line: continuum spectrum including the narrow iron Kα emission line and the black body. Purple line: relativistically smeared reflection component. Second panel: measured count rate spectra. The four lowest panels show the best fit residuals for observations Obs1–Obs4. EPIC-pn is blue, PCA is red, HEXTE is green and ISGRI is orange.
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