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Fig. 13

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The effect of a poor estimation of the Galactic diffuse emission. The histograms are the p- value distributions for the Cygnus field when the null hypothesis for Cygnus X-3 is true with the following parameters: Tss = 4, tlcl = 5.99147, flux and position of Cygnus X-3 left free. The true value of giso in the simulated data is 7.7, the value of ggal used in the analysis is fixed to 0.67. Blue thin line: simulated ggal = 0.67, giso fixed to 7.7; blue thick line: simulated ggal = 0.67, gisoleft free; red thick line: simulated ggal = 0.67 ∗ 1.1, gisoleft free; black thick line: simulated ggal = 0.67 ∗ 0.89, gisoleft free. The red dotted line is the theoretical distribution, the green dashed line is the theoretical distribution, the cyan dotted-dashed line is the distribution.

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