Abstract
The Sculptor and Carina dwarf spheroidal galaxies were observed with the H.E.S.S. Cherenkov telescope array between January 2008 and December 2009. The data sets consist of a total of 11.8 h and 14.8 h of high quality data, respectively. No gamma-ray signal was detected at the nominal positions of these galaxies above 220 GeV and 320 GeV, respectively. Upper limits on the gamma-ray fluxes at 95% CL assuming two forms for the spectral energy distribution (a power law shape and one derived from dark matter annihilation) are obtained at the level of 10-13-10-12 cm-2 s-1 in the TeV range. Constraints on the velocity weighted dark matter particle annihilation cross section for both Sculptor and Carina dwarf galaxies range from 〈σv〉 ∼ 10-21 cm3 s-1 down to 〈σv〉 ∼ 10-22 cm3 s -1 depending on the dark matter halo model used. Possible enhancements of the gamma-ray flux are studied: the Sommerfeld effect, which is found to exclude some dark matter particle masses, the internal Bremsstrahlung and clumps in the dark-matter halo distributions.
| Original language | English |
|---|---|
| Pages (from-to) | 608-616 |
| Number of pages | 9 |
| Journal | Astroparticle Physics |
| Volume | 34 |
| Issue number | 8 |
| DOIs | |
| Publication status | Published - 1 Jan 2011 |
Keywords
- Carina
- Dark matter
- Gamma-rays: observations - Dwarf spheroidal galaxy
- Internal Bremsstrahlung
- Sculptor
- Sommerfeld enhancement