Spectral analysis of the gamma-ray background near the dwarf Milky Way satellite Segue 1: Improved limits on the cross section of neutralino dark matter annihilation
Journal Article
·
· Physical Review. D, Particles, Fields, Gravitation and Cosmology
- Univ. of Potsdam (Germany). Inst. of Physics and Astronomy
The indirect detection of dark matter requires that dark matter annihilation products be discriminated from conventional astrophysical backgrounds. We re-analyze GeV-band gamma-ray observations of the prominent Milky Way dwarf satellite galaxy Segue 1, for which the expected astrophysical background is minimal. Here, we explicitly account for the angular extent of the conservatively expected gamma-ray signal and keep the uncertainty in the dark-matter profile external to the likelihood analysis of the gamma-ray data.
- Research Organization:
- SLAC National Accelerator Lab., Menlo Park, CA (United States)
- Sponsoring Organization:
- USDOE
- Grant/Contract Number:
- AC02-76SF00515
- OSTI ID:
- 1356671
- Journal Information:
- Physical Review. D, Particles, Fields, Gravitation and Cosmology, Vol. 86, Issue 6; ISSN 1550-7998
- Publisher:
- American Physical Society (APS)Copyright Statement
- Country of Publication:
- United States
- Language:
- English
Cited by: 13 works
Citation information provided by
Web of Science
Web of Science
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Indication of Gamma-ray Emission from the Newly Discovered Dwarf Galaxy Reticulum II | text | January 2018 |
Indication of Gamma-ray Emission from the Newly Discovered Dwarf Galaxy Reticulum II
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A Comprehensive Search for Dark Matter Annihilation in Dwarf Galaxies | text | January 2014 |
A Global Analysis of Dark Matter Signals from 27 Dwarf Spheroidal Galaxies using 11 Years of Fermi-LAT Observations | text | January 2018 |
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