Fig. 5.
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Histogram of the angular difference between the jet and the X-ray PA, computed for every HSP observation. Mrk 421 (yellow dashed line) and 1ES 1959+650 (blue dash-dotted line) are plotted separately from the others, as they present large amplitude rotations of the PA during the IXPE observation periods. The other sources are plotted altogether (red solid line).
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