Recycling serendipitous observations of XRISM for dark matter searches
astro-ph.HE
Submitted: 2026-10-01
Updated: 2026-10-01
Terminology
Sources
- Direct Detection of Warm Dark Matter in the X-ray
- Where to find a dark matter sterile neutrino?
- Sterile Neutrino Dark Matter
- The search for decaying Dark Matter
- Chandra X-Ray Observatory (CXO):Overview
- Detection of An Unidentified Emission Line in the Stacked X-ray spectrum of Galaxy Clusters
- An unidentified line in X-ray spectra of the Andromeda galaxy and Perseus galaxy cluster
- Checking the dark matter origin of 3.53 keV line with the Milky Way center
- Testing the origin of ~3.55 keV line in individual galaxy clusters observed with XMM-Newton
- Radial Profile of the 3.55 keV line out to $R_{200}$ in the Perseus Cluster
- A Suzaku Search for Dark Matter Emission Lines in the X-ray Brightest Galaxy Clusters
- Decaying dark matter search with NuSTAR deep sky observations
- Searching for the 3.5 keV Line in the Deep Fields with Chandra: the 10 Ms observations
- Surface brightness profile of the 3.5 keV line in the Milky Way halo
- 7.1 keV sterile neutrino dark matter constraints from a deep Chandra X-ray observation of the Galactic bulge Limiting Window
- Sterile neutrino dark matter bounds from galaxies of the Local Group
- Constraints on 3.55 keV line emission from stacked observations of dwarf spheroidal galaxies
- Questioning a 3.5 keV dark matter emission line
- An X-ray Spectroscopic Search for Dark Matter in the Perseus Cluster with Suzaku
- Searching for keV Sterile Neutrino Dark Matter with X-ray Microcalorimeter Sounding Rockets
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