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Fig. 10

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‘’Data-space” method applied to V0332+53. The source intensity variations (25–50 keV) were modeled by nine segments (red) and were compared with the IBIS time series (26–51 keV, gray). The green curve corresponds to the IBIS flux averaged on SPI-obtained segments. The insert is a zoom between exposure number 81 and 179. (Top) SPI intensity variations model (black) compared with Swift/BAT time series (24–50 keV, purple line). The scale between the different instruments is arbitrary and was chosen such that their measured total fluxes are equal. It should be noted that the Swift/BAT and IBIS data are not necessarily recorded at the same time as the SPI data, nor exactly in the same energy band.

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