PreprintarXiv licencearXiv
Recycling serendipitous observations of XRISM for dark matter searches
Abstract
Searches for radiative decays of keV-mass dark matter have been limited by energy resolution. We propose a strategy for the XRISM/Resolve low count rate observations, and search the 3.48-3.56 keV band for a decay line from the Milky Way halo. Despite a lower exposure, our bounds are stronger than those from XRISM observations of galaxy clusters. We also identify a residual at E = 3.5311 keV with ~3sigma local significance, coincident with the previously reported unidentified feature, and having no plausible atomic or instrumental counterpart. These bounds will continue to tighten as additional pointings become available.
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BibTeX
@misc{zadorozhna2026recycling,
title = {{Recycling serendipitous observations of XRISM for dark matter searches}},
author = {Lidiia Zadorozhna and Denys Malyshev and Oleg Ruchayskiy},
howpublished = {arXiv},
year = {2026},
month = oct,
doi = {10.48550/arxiv.2610.01877},
eprint = {2610.01877},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2610.01877},
}
RIS
TY - UNPB
TI - Recycling serendipitous observations of XRISM for dark matter searches
AU - Lidiia Zadorozhna
AU - Denys Malyshev
AU - Oleg Ruchayskiy
PY - 2026
DA - 2026/10/01
PB - arXiv
DO - 10.48550/arxiv.2610.01877
UR - https://arxiv.org/abs/2610.01877
AB - Searches for radiative decays of keV-mass dark matter have been limited by energy resolution. We propose a strategy for the XRISM/Resolve low count rate observations, and search the 3.48-3.56 keV band for a decay line from the Milky Way halo. Despite a lower exposure, our bounds are stronger than those from XRISM observations of galaxy clusters. We also identify a residual at E = 3.5311 keV with ~3sigma local significance, coincident with the previously reported unidentified feature, and having no plausible atomic or instrumental counterpart. These bounds will continue to tighten as additional pointings become available.
ER -