UCL Discovery Stage
UCL home » Library Services » Electronic resources » UCL Discovery Stage

Searching for Dark Matter Annihilation in Recently Discovered Milky Way Satellites with Fermi-LAT

Albert, A; Anderson, B; Bechtol, K; Drlica-Wagner, A; Meyer, M; Sánchez-Conde, M; Strigari, L; ... Walker, AR; + view all (2017) Searching for Dark Matter Annihilation in Recently Discovered Milky Way Satellites with Fermi-LAT. Astrophysical Journal , 834 (2) , Article 110. 10.3847/1538-4357/834/2/110. Green open access

[thumbnail of Albert_2017_ApJ_834_110.pdf]
Preview
Text
Albert_2017_ApJ_834_110.pdf - Published Version

Download (2MB) | Preview

Abstract

© 2017. The American Astronomical Society. All rights reserved.We search for excess γ-ray emission coincident with the positions of confirmed and candidate Milky Way satellite galaxies using six years of data from the Fermi Large Area Telescope (LAT). Our sample of 45 stellar systems includes 28 kinematically confirmed dark-matter-dominated dwarf spheroidal galaxies (dSphs) and 17 recently discovered systems that have photometric characteristics consistent with the population of known dSphs. For each of these targets, the relative predicted γ-ray flux due to dark matter annihilation is taken from kinematic analysis if available, and estimated from a distance-based scaling relation otherwise, assuming that the stellar systems are DM-dominated dSphs. LAT data coincident with four of the newly discovered targets show a slight preference (each ∼2σ local) for γ-ray emission in excess of the background. However, the ensemble of derived γ-ray flux upper limits for individual targets is consistent with the expectation from analyzing random blank-sky regions, and a combined analysis of the population of stellar systems yields no globally significant excess (global significance < 1σ). Our analysis has increased sensitivity compared to the analysis of 15 confirmed dSphs by Ackermann et al. The observed constraints on the DM annihilation cross section are statistically consistent with the background expectation, improving by a factor of ∼2 for large DM masses (mDM,bb ≳ 1 TeV and mDM,τ+τ- ≳70 GeV) and weakening by a factor of ∼1.5 at lower masses relative to previously observed limits.

Type: Article
Title: Searching for Dark Matter Annihilation in Recently Discovered Milky Way Satellites with Fermi-LAT
Open access status: An open access version is available from UCL Discovery
DOI: 10.3847/1538-4357/834/2/110
Publisher version: http://dx.doi.org/10.3847/1538-4357/834/2/110
Additional information: © 2017. The American Astronomical Society. All rights reserved
Keywords: dark matter; galaxies: dwarf; gamma rays: galaxies
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy
URI: https://discovery-pp.ucl.ac.uk/id/eprint/1540815
Downloads since deposit
1,771Downloads
Download activity - last month
Download activity - last 12 months
Downloads by country - last 12 months

Archive Staff Only

View Item View Item