The Fermi LAT collaboration has recently presented constraints on the gamma-ray signal from annihilating dark matter using separate analyses of a number of dwarf spheroidal galaxies. Since the expected annihilation signal has the same physical properties regardless of the target (except for a normalization scale), it is possible to enhance the constraining power using a combined analysis, the initial results of which will be presented here. © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence.
CITATION STYLE
Garde, M. L. (2010). Constraining dark matter signal from a combined analysis of Milky Way satellites using the Fermi-LAT. In Proceedings of Science. https://doi.org/10.22323/1.110.0116
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