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Fig. 2

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200 MeV−20 GeV residual counts maps after subtraction of the fitted celestial background model and a smoothing with a 2D Gaussian kernel with σ = 0.4°. Upper plot corresponds to the full region of interest and lower plot is a zoom on the SMC. The positions of the background point sources are marked by white circles in the top panel, with circle size indicating position uncertainty, and the SMC is traced by H I column density contours in the bottom panel.

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