30 citations · 30 across the 3 of their papers we have counts for
3 papers
astro-ph.IM2019
Revisiting the expected Micro-X signal from the 3.5 keV line
Denys Savchenko, Dmytro Iakubovskyi
One of the future instruments to resolve the origin of the unidentified 3.5 keV emission line is the Micro-X sounding rocket telescope. According to the estimate made in 2015, Micr…
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…