794 citations · 3.6k across the 49 of their papers we have counts for
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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…
Multi-wavelength analysis of the Galactic supernova remnant MSH 11-61A
Katie Auchettl, Patrick Slane, Daniel Castro +2
Due to its centrally bright X-ray morphology and limb brightened radio profile, MSH 11-61A (G290.1-0.8) is classified as a mixed morphology supernova remnant (SNR). H$\textsc{i}$ a…
A Chandrasekhar Mass Progenitor for the Type Ia Supernova Remnant 3C 397 from The Enhanced Abundances of Nickel and Manganese
Hiroya Yamaguchi, Carles Badenes, Adam R. Foster +8
Despite decades of intense efforts, many fundamental aspects of Type Ia supernova (SNe Ia) remain elusive. One of the major open questions is whether the mass of the exploding whit…