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Surface brightness profile of the 3.5 keV line in the Milky Way halo

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arxiv 1812.10488 v2 pith:IO4JIKUO submitted 2018-12-26 astro-ph.HE hep-ph

A. Boyarsky , D. Iakubovskyi , O. Ruchayskiy , D. Savchenko This is my paper · ORCID
classification astro-ph.HEhep-ph
keywords linemilkycompareobservationsprofileangularastrophysicalbounds
verification ladder T0 review T1 audit T2 compute T3 formal
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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.

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Cited by 1 Pith paper

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    astro-ph.IM 2025-05 conditional novelty 6.0 of 10

    A mission design paper describing how a skipper-CCD CubeSat in low Earth orbit could search for strongly interacting sub-GeV dark matter and decaying dark matter X-rays.

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