Fig. 3.
Magnified view of the December 2017 outburst seen by OGLE (red points). Superimposed are the 0.3−8 keV fluxes from the Swift/XRT monitoring of AXJ0049.4–7323 (blue points), and the times of the AAT observations (green bars). The grey vertical dashed line shows the expected time of the peak of the optical outburst calculated with the ephemeris of Schmidtke et al. (2013).
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