Limits to Dark Matter Annihilation Cross-Section from a Combined Analysis of MAGIC and Fermi-LAT Observations of Dwarf Satellite Galaxies
Jan 25, 201619 pages
Published in:
- JCAP 02 (2016) 039
- Published: Feb 16, 2016
e-Print:
- 1601.06590 [astro-ph.HE]
Report number:
- FERMILAB-PUB-16-283-AE
Citations per year
Abstract: (IOP)
We present the first joint analysis of gamma-ray data from the MAGIC Cherenkov telescopes and the Fermi Large Area Telescope (LAT) to search for gamma-ray signals from dark matter annihilation in dwarf satellite galaxies. We combine 158 hours of Segue 1 observations with MAGIC with 6-year observations of 15 dwarf satellite galaxies by the Fermi-LAT. We obtain limits on the annihilation cross-section for dark matter particle masses between 10 GeV and 100 TeV—the widest mass range ever explored by a single gamma-ray analysis. These limits improve on previously published Fermi-LAT and MAGIC results by up to a factor of two at certain masses. Our new inclusive analysis approach is completely generic and can be used to perform a global, sensitivity-optimized dark matter search by combining data from present and future gamma-ray and neutrino detectors.Note:
- 19 pages, 3 figures. V2: Few typos corrected and references added. Matches published version JCAP 02 (2016) 039
- dark matter experiments
- gamma ray experiments
- dwarfs galaxies
- neutrino experiments
- dark matter: annihilation
- cross section: annihilation
- neutrino: detector
- gamma ray: VHE
- MAGIC
- satellite
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Figures(3)
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