A deep spectromorphological study of the γ-ray emission surrounding the young massive stellar cluster Westerlund 1

Open Access

Fig. A.2.

Flux maps after subtraction of Galactic diffuse γ-ray emission. The maps are the same as in Fig. 3, except that the Galactic diffuse γ-ray flux as predicted by the PICARD code has been subtracted. The colour axis scales and flux levels of contour lines are identical to those in Fig. 3.

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