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astro-ph.HE2015
Identification of the ~3.55 keV emission line candidate objects across the sky
Denys Savchenko, Dmytro Iakubovskyi
Emission line at the energy ~3.55 keV detected in different galaxies and galaxy clusters has caused a lot of discussion in high-energy astrophysics and particle physics communities…
astro-ph.HE2015★ 30 cited
Testing the origin of ~3.55 keV line in individual galaxy clusters observed with XMM-Newton
Dmytro Iakubovskyi, Esra Bulbul, Adam R. Foster +2
If the unidentified emission line at ~3.55 keV previously found in spectra of nearby galaxies and galaxy clusters is due to radiatively decaying dark matter, one should detect the…