Fig. 3
Estimated most probable spin frequencies of RX J0720.4−3125 (for details, see text and Table 2) obtained by application of the GL method for periodicity searching in the broad energy band for ObsIds 0124100101 and 0164560501 (XMM-Newton EPIC-pn Full Frame mode). The highest posterior density (HPD) intervals, 68% and 95%, are determined as a probabilistic region around a posterior mode and depicted as vertical dashed lines in black and red, respectively.
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