Fig. A.1.
XMM-Newton EPIC pn light curve of the central star in IRAS 00500+6713. The light-curve was background corrected and binned by 600 s; the error bars correspond to 3σ. The Y-axis is the time after the start of the observation. Black and blue data points refer to the first and second observation, respectively (see Table A.1). For the second observation, the X-axis is shifted by 15 000 s for clarity.
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