Fig. 5.
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Timing analysis of XMM-Newton observation 0303420201. Top figure: PN+MOS light curve of ULX-7. The bin time is 100 s, as in the three LP light curves. Bottom figure: ULX-7 PDS in the 0.3–10 keV band (top panel) and residuals of the white noise plus single Lorentzian model used for this observation (bottom panel). We combined data from PN and MOS cameras. The PDS is computed using the Leahy normalization.
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