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Fig. 1.


Background-subtracted light curve of J0331−27 in the 0.2–2 keV energy range combining pn and MOS data. A 30 ks portion of the observation is shown. Count rate has been converted to flux in the 0.5–2 keV energy range using the best fit spectral model (see text). The flare from the source is apparent, and is nicely described by a linear rise and exponential decay model (see text).

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