Extended Data Fig. 1: The stellar density templates for the Sgr dSph used in this study.
From: Gamma-ray emission from the Sagittarius dwarf spheroidal galaxy due to millisecond pulsars
Each map has been normalized, so the units are arbitrary; the color scale is logarithmic. Morphological differences among the templates are due to different stellar candidates (red clump or RR Lyrae), search algorithms, and search target (the dwarf remnant or the stream). Data sources are as follows: Model I, ref. 8; Model II, ref. 39; Model III, ref. 40; Model IV and Model V, ref. 41. Detailed descriptions of these templates are given in the S.I. sec. 2.
