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Volume 358 - 36th International Cosmic Ray Conference (ICRC2019) - DM - Dark Matter
Searching for Dark Matter decay signals in the Galactic halo with the MAGIC telescopes
D. Ninci,* T. Inada, J. Rico, D. Kerszberg, M. Doro, S. Lombardi, C. Maggio, M. Hütten, M.V. Acosta
*corresponding author
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Pre-published on: 2019 July 22
Published on:
Abstract
MAGIC is a system of two Cherenkov telescopes located in the Canary island of La Palma. A key part of MAGIC Fundamental Physics program is the search for indirect signals of Dark Matter (DM) from different sources. In the Milky Way, DM forms an almost spherically symmetric halo, with a density peaked towards the center of the Galaxy and decreasing toward the outer region. We search for DM decay signals from the Galactic Halo, with a special methodology developed for this work. Our strategy is to compare pairs of observations performed at different angular distances from the Galactic Center, selected in such a way that all the diffuse components cancel out, except for those coming from the DM. In order to keep the systematic uncertainty of this novel background estimation method down to a minimum, the observation pairs have been acquired during the same nights and follow exactly the same azimuth and zenith paths. We collected 20 hours of data during 2018. Using half of them to determine the systematic uncertainty in the background estimation of our analysis, we obtain a value of 4.8% with no dependence on energy. Accounting for this systematic uncertainty in the likelihood analysis based on the 10 remaining hours of data collected so far, we present the limit to TeV DM particle with a lifetime of 10^26 s in
the bb̄ decay channel.
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