Fig. 2: The second eROSITA QPE.
From: X-ray quasi-periodic eruptions from two previously quiescent galaxies
a, b, As in Fig. 1a, b, for eRO-QPE2. The start of the eROSITA light curve is approximately MJD 59023.191. c, As in Fig. 1c, for the XMM-Newton observation of eRO-QPE2. tXMM,1 corresponds to the start of the cleaned MOS1 exposure, approximately MJD 59067.846. The mean (and related dispersion) of the rise-to-decay duration is about 27 min (~3 min), with a peak-to-peak separation of approximately 2.4 h (~5 min). All uncertainties are 1σ, shown as error bars or shaded regions.
