Broadband spectral energy distribution. Emission from the central 10′ around V4641 Sgr is shown (coincident MeerKAT and XRISM detections), together with Fermi-LAT, H.E.S.S., HAWC and LHAASO spectra (Suzuki et al. 2025; Neronov et al. 2025; H.E.S.S. Collaboration 2025; Alfaro et al. 2024; LHAASO Collaboration 2025) at larger scales (∼1°). The gray points correspond to gamma-ray fluxes, scaled down to the XRISM source region by relative area. Synchrotron and IC models (dotted lines), as well as the pion decay model (black solid line) are overlaid.