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Title: 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

Abstract

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.

Authors:
 [1];  [1];  [1]
  1. Univ. of Potsdam (Germany). Inst. of Physics and Astronomy
Publication Date:
Research Org.:
SLAC National Accelerator Lab., Menlo Park, CA (United States)
Sponsoring Org.:
USDOE
OSTI Identifier:
1356671
Grant/Contract Number:  
AC02-76SF00515
Resource Type:
Journal Article: Accepted Manuscript
Journal Name:
Physical Review. D, Particles, Fields, Gravitation and Cosmology
Additional Journal Information:
Journal Volume: 86; Journal Issue: 6; Journal ID: ISSN 1550-7998
Publisher:
American Physical Society (APS)
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS

Citation Formats

Baushev, A. N., Federici, S., and Pohl, M. 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. United States: N. p., 2012. Web. doi:10.1103/PhysRevD.86.063521.
Baushev, A. N., Federici, S., & Pohl, M. 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. United States. https://doi.org/10.1103/PhysRevD.86.063521
Baushev, A. N., Federici, S., and Pohl, M. 2012. "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". United States. https://doi.org/10.1103/PhysRevD.86.063521. https://www.osti.gov/servlets/purl/1356671.
@article{osti_1356671,
title = {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},
author = {Baushev, A. N. and Federici, S. and Pohl, M.},
abstractNote = {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.},
doi = {10.1103/PhysRevD.86.063521},
url = {https://www.osti.gov/biblio/1356671}, journal = {Physical Review. D, Particles, Fields, Gravitation and Cosmology},
issn = {1550-7998},
number = 6,
volume = 86,
place = {United States},
year = {Thu Sep 20 00:00:00 EDT 2012},
month = {Thu Sep 20 00:00:00 EDT 2012}
}

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Free Publicly Available Full Text
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Cited by: 13 works
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Works referenced in this record:

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journal, June 2009


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Works referencing / citing this record:

A global analysis of dark matter signals from 27 dwarf spheroidal galaxies using 11 years of Fermi-LAT observations
journal, February 2020


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
text, January 2015


A Comprehensive Search for Dark Matter Annihilation in Dwarf Galaxies
text, January 2014