Fig. 17

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Differential sensitivity of LST-1 using the likelihood reconstruction method in percentage of the Crab Nebula flux. This was obtained from data by optimizing the gammaness and angular cuts for best sensitivity. The sensitivity shown here for the likelihood reconstruction, and associated statistical errors, are the average of the curves obtained through reversing the half of events used for cut optimization and sensitivity estimation. The “standard” sensitivity is from Abe et al. (2023).
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