Titlebook: Optimized Dark Matter Searches in Deep Observations of Segue 1 with MAGIC; Jelena Aleksi? Book 2016 Springer International Publishing Swit

Ascendancy

聯(lián)想

Jelena Aleksi?Nominated as an outstanding Ph.D. thesis by the Institut de Física d‘Altes Energies, Spain.Presents the deepest survey of dwarf spheroidal galaxy Segue 1.Outlines the analysis optimized for dark matte

guardianship

The MAGIC Telescopes,gies and fast response to variable phenomena. This chapter is devoted to the description of technical properties of the MAGIC Telescopes, as well as of the standard observational procedures and of the analysis chain used to process the gathered data.

漫步

Calculus

Dark Matter Searches,t to catch a glimpse of the elusive dark matter particle, however, to date, no undeniable results can be claimed. Based on the approach, three main detection techniques can be distinguished: production of dark matter in particle accelerators, direct detection through dark matter scattering off ordin

Neutropenia

The MAGIC Telescopes,gies and fast response to variable phenomena. This chapter is devoted to the description of technical properties of the MAGIC Telescopes, as well as of the standard observational procedures and of the analysis chain used to process the gathered data.

sigmoid-colon

Full Likelihood Method,mma-ray sources to probing some of the most intriguing questions of the fundamental physics and cosmology. However, their standard analysis tools and methods are adapted for detection of power law-like signals from astrophysical objects of conventional origin, at the expense of sources whose emissio

GLOOM

Dark Matter Searches in Dwarf Spheroidal Galaxy Segue 1 with MAGIC,carried out with the MAGIC Telescopes between January 2011 and February 2013. With 157.9?h of good-quality data, this is the deepest survey of any dwarf galaxy by any IACT so far. Here are described the motivation behind the choice of Segue 1 as a suitable dark matter target, details of its observat

不整齊

Future Prospects,ulation of additional hours no longer increases the sensitivity, and the energy and angular resolution of the telescopes cannot be improved any further. Fortunately, progress towards the future of Cherenkov astronomy is already well under way: the Cherenkov Telescope Array (CTA) will mark the new ge

nonplus

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