Image Details
Caption: Figure C3.
The profile of the TS of the fit improvement when a Gaussian disk with Gaussian radius of 0﹩\mathop{.}\limits^{{\unicode{x000b0}}}﹩00–1﹩\mathop{.}\limits^{{\unicode{x000b0}}}﹩00 was considered for the GRS 1915+105–LHAASO counterpart.
© 2026. The Author(s). Published by the American Astronomical Society.