Fig. 8.

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From top to bottom: evolution of the photon index (measured using the Mpl model), ratio of the f0.2 − 2.0 keV to the 2246 Å monochromatic flux, apparent UVM2 AB magnitude, and log(f0.2 − 2.0 keV) against the time offset. The time off-set is calculated relative to the inferred t0 assuming a period of 223 days. The whole data set was split into three cycles that were determined by the time when the rapid X-ray flux drop occurred. The vertical dashed lines represent the time (relative to t0 of each cycle) of the ATCA radio observations. Radio emission was detected only in cycle 3 (dashed blue lines).

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