Fig. 6
Unfolded spectrum of IGR J12580+0134 from Swift observations made in PC mode (top) and unfolded XMM-Newton/Epic-pn and INTEGRAL/ISGRI spectra (bottom). The best-fit model (an absorbed power law in all spectra plus an unabsorbed black-body emission below 1 keV in case of Epic-pn observation) is shown by solid lines in both upper panels. Lower panels indicate the residuals (Δχ).
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