The SVOM/ECLAIRs image trigger with wavelet-based background correction optimised with a one-year simulation of observations

Open Access

Fig. 4

Distribution of the S/N in 20 min sky images for different combinations of the filter size and the maximum scale used for the wavelet cleaning. The black solid curve corresponds to the normal distribution. The best parameters (h₃, s_th = 3) are shown as the solid green curve.

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