{ "id": "1605.02793", "version": "v1", "published": "2016-05-09T21:40:01.000Z", "updated": "2016-05-09T21:40:01.000Z", "title": "Prospects for annihilating Dark Matter towards Milky Way's dwarf galaxies by the Cherenkov Telescope Array", "authors": [ "Valentin Lefranc", "Paolo Panci", "Gary A. Mamon" ], "comment": "16 pages, 4 figures", "categories": [ "astro-ph.HE", "hep-ex", "hep-ph" ], "abstract": "We derive the large Cherenkov Telescope Array (CTA) sensitivity to dark matter (DM) annihilation in several primary channels, over a broad range of DM masses. These sensitivities are estimated when CTA is pointed towards a large sample of Milky Way's dwarf spheroidal galaxies (dSphs) with promising $J$-factors and small statistical uncertainties. This analysis neglects systematic uncertainties, which we estimate at the level of at least 1 dex. We also present sensitivities on the annihilation cross section from a combined analysis of 4 dSphs. We assess the CTA sensitivity by: $i)$ using, for each dSph, recent determination of the $J$-factor and its statistical error; $ii)$ considering the most up-to-date cosmic ray background; and $iii)$ applying a joint spatial and spectral analysis in the likelihood. We find that a joint spectral and spatial analysis improves the CTA sensitivity, in particular for primary channels with sharp features in the $\\gamma$-ray energy spectrum and for dSphs with steep $J$-factor profiles, as deduced from the internal kinematics. The greatest sensitivities are obtained for observations of Ursa Minor among the classical dSphs and of Ursa Major II for ultra-faint dSphs.", "revisions": [ { "version": "v1", "updated": "2016-05-09T21:40:01.000Z" } ], "analyses": { "keywords": [ "cherenkov telescope array", "milky ways dwarf galaxies", "annihilating dark matter", "ways dwarf spheroidal galaxies", "sensitivity" ], "note": { "typesetting": "TeX", "pages": 16, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1456908 } } }