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Fig. 8
IBIS/ISGRI light curve in response to different spectral models. Dashed lines represent the temporal evolution of the 144.5−168 keV band of the 3Dbball, DDT1p4, and W7 models (from top to bottom) multiplied by the effective area in this band (370 cm2). Continuous lines represent their convolution with the ISGRI response.
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