A. Boyarsky, D. Iakubovskyi, O. Ruchayskiy, D. Savchenko
Published 2018-12-26Version 1
We report a detection of 3.5 keV line in the Milky Way in 5 regions offset from the Galactic Center by distances from 10' to 35 degrees. We build an angular profile of this line and compare it with profiles of several astrophysical lines detected in the same observations. We compare our results with other detections and bounds previously obtained using observations of the Milky Way.
Discovery of a 3.5 keV line in the Galactic Center and a Critical Look at the Origin of the Line Across Astronomical Targets
Analyzing γ-rays of the Galactic Center with Deep Learning
Hunting for Heavy Winos in the Galactic Center
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