SARAS3 data sets T21 ≳ -277.6 mK at z=23.6 (3σ) in IDM models and finds no preference for IDM over CDM (Bayes factor ≈1.7).
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No dark matter annihilation signal is detected from dwarf galaxies; upper limits on the velocity-weighted cross-section are set at order 10^{-23} cm^3 s^{-1} for DM masses 1-10^4 TeV.
citing papers explorer
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Implications of \textit{SARAS3} data for Coulomb-like interacting dark matter
SARAS3 data sets T21 ≳ -277.6 mK at z=23.6 (3σ) in IDM models and finds no preference for IDM over CDM (Bayes factor ≈1.7).
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Improved Heavy Dark Matter Annihilation Search from Dwarf Galaxies with HAWC
No dark matter annihilation signal is detected from dwarf galaxies; upper limits on the velocity-weighted cross-section are set at order 10^{-23} cm^3 s^{-1} for DM masses 1-10^4 TeV.