Speaker
Sytov, Alexei
(Universita e INFN, Ferrara (IT))
Description
Dwarf galaxies have long been considered an ideal target in the search of annihilation from wimp-like dark matter particles. As has been shown by Fermi, few dwarf galaxies have shown indications of an excess at the 3-4 sigma, typically limited by the amplitude of the background, and the angular resolution of the detector. I will discuss the advantages of a pencil-like detector approach in the search for a signal from dwarf galaxies and demonstrate the advantages and utility of such technologies in other faint astrophysical sources.
| Eligibility for "Best presentation for young researcher" prize | No |
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Authors
Bandiera, Laura
(Universita e INFN, Ferrara (IT))
Gaitskell, Richard
Koushiappas, Savvas
Koushiappas, Savvas
(Brown University)
Soldani, Mattia
(Università degli Studi dell'Insubria & INFN Milano Bicocca)
Sytov, Alexei
(Universita e INFN, Ferrara (IT))
