Fig. 1.
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θ2 plot on SGR 1935+2154 persistent emission. We used 25.5 h of high-quality data (see Sect. 3), which we show here in a single energy bin from 0.1 TeV to 10 TeV. We show the distribution of ON counts in blue and the background distribution in orange. The dashed line represents the θ2 cut used to evaluate the significance. No emission is detected.
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