Fig. 11
1AGLR J2033+4057/Cyg X-3 E > 100 MeV light curve (upper panel) compared with the Swift/BAT 15 < E < 150 keV daily light curve. The plot shows six detections with 
. The 1−2 days γ-ray flare times described in Tavani et al. (2009c), Bulgarelli et al. (2012a), and Piano et al. (2012) are marked with vertical magenta lines. For some lines there is no corresponding UL when they have 
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