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Fig. 7

image

Long-term BAT lightcurve of Swift J1734.5-3027 in the 1550 keV energy range. The two outbursts of the source in MayJune 2013 (red points) and September 2013 (green and cyan points) are clearly visible. For the outburst in September, we highlighted in green the initial part of the event up to the quiescent period around 56 545 MJD. The cyan points mark the re-brightening of the source after the quiescent period up to 56 614 MJD. Gaps in the BAT lightcurve are due to the source proximity to the Sun.

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