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Fig. 4
Outburst evolution of the best-fit spectral parameters of the compps model using the RXTE/PCA/HEXTE data in the 2.5–200 keV range. Each spectrum corresponds to one RXTE observation of IGR J17511–3057. The bolometric luminosity is given in the energy range 0.5–200 keV assuming a source distance of 7 kpc.
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