Where do the 3.5 keV photons come from? A morphological study of the Galactic Center and of Perseus
Authors:
- Eric CarlsonECEric Carlson
- Tesla JeltemaTJTesla Jeltema
- Stefano ProfumoStefano Profumo
- 1 February 2015
- journal article
- Published by IOP Publishing in Journal of Cosmology and Astroparticle Physics
- Vol. 2015 (02) , 009
Abstract
No abstract availableKeywords
All Related Versions
This publication has 30 references indexed in Scilit:
- Unidentified Line in X-Ray Spectra of the Andromeda Galaxy and Perseus Galaxy ClusterPhysical Review Letters, 2014
- Constraints on 3.55 keV line emission from stacked observations of dwarf spheroidal galaxiesPhysical Review D, 2014
- Cluster X-ray line at $3.5~\mathrm{keV}$ 3.5 keV from axion-like dark matterThe European Physical Journal C, 2014
- 3.55 keV photon line and its morphology from a 3.55 keV axionlike particle linePhysical Review D, 2014
- DETECTION OF AN UNIDENTIFIED EMISSION LINE IN THE STACKED X-RAY SPECTRUM OF GALAXY CLUSTERSThe Astrophysical Journal, 2014
- The 7 keV axion dark matter and the X-ray line signalPhysics Letters B, 2014
- 3.55 keV hint for decaying axionlike particle dark matterPhysical Review D, 2014
- The Role of Sterile Neutrinos in Cosmology and AstrophysicsAnnual Review of Nuclear and Particle Science, 2009
- SimultaneousChandra, CSO, and VLA Observations of Sgr A*: The Nature of Flaring ActivityThe Astrophysical Journal, 2008
- A DeepChandraCatalog of X‐Ray Point Sources toward the Galactic CenterThe Astrophysical Journal, 2003