
A Search for the 3.5 keV Line from the Milky Way's Dark Matter Halo with HaloSat
We use HaloSat observations of the Milky Way's Galactic dark matter halo to search for a 3.5 keV X-ray emission line associated with the decay of a 7.1 keV sterile neutrino dark matter candidate. Reporting a non-detection, we place upper limits on the 3.5 keV line flux and the corresponding 7.1 keV sterile neutrino mixing angle.