Fig. 3.
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Joint spectropolarimetric analysis of 1ES 1101-232. Left: Energy flux spectra, expressed as photon flux multiplied by energy squared, for the Swift (red), IXPE I (yellow), and NuSTAR (blue) data together with the corresponding data-model residuals. The black line indicates the best-fit model. Right: IXPE Q and U spectra, displayed in green and orange, respectively, together with their deviations from the best-fit model.
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