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Optimized Dark Matter Searches in Deep Observations of Segue 1 with MAGIC (Hardcover, 1st ed. 2016)
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Optimized Dark Matter Searches in Deep Observations of Segue 1 with MAGIC (Hardcover, 1st ed. 2016)
Series: Springer Theses
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This thesis presents the results of indirect dark matter searches
in the gamma-ray sky of the near Universe, as seen by the MAGIC
Telescopes. The author has proposed and led the 160 hours long
observations of the dwarf spheroidal galaxy Segue 1, which is the
deepest survey of any such object by any Cherenkov telescope so
far. Furthermore, she developed and completely characterized a new
method, dubbed "Full Likelihood", that optimizes the sensitivity of
Cherenkov instruments for detection of gamma-ray signals of dark
matter origin. Compared to the standard analysis techniques, this
novel approach introduces a sensitivity improvement of a factor of
two (i.e. it requires 4 times less observation time to achieve the
same result). In addition, it allows a straightforward merger of
results from different targets and/or detectors. By selecting the
optimal observational target and combining its very deep exposure
with the Full Likelihood analysis of the acquired data, the author
has improved the existing MAGIC bounds to the dark matter
properties by more than one order of magnitude. Furthermore, for
particles more massive than a few hundred GeV, those are the
strongest constraints from dwarf galaxies achieved by any gamma-ray
instrument, both ground-based or space-borne alike.
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