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DTSTART;TZID=Europe/Rome:20170606T114500
DTEND;TZID=Europe/Rome:20170606T124500
DTSTAMP:20260405T142254
CREATED:20170412T103150Z
LAST-MODIFIED:20170412T103150Z
UID:2849-1496749500-1496753100@www.oa-roma.inaf.it
SUMMARY:Dwarf spheroidal satellite galaxies under the eye of Cherenkov telescopes: indirect search for dark matter by MAGIC and opportunities and prospects for CTA
DESCRIPTION:Searching for gamma-ray signals from dark matter annihilation in dwarf\nspheroidal satellite galaxies (dSphs) of the Milky Way plays a critical\nrole within the framework of indirect dark matter searches. This study\,\naimed at unveiling the nature of the most elusive component of the\nUniverse\, is potentially able to confirm the dark matter interpretation of\nthe observed gamma-ray excess in the Galactic Center.\nThanks to deep observation campaigns on dSphs\, MAGIC achieved stringent\nconstraints to dark matter annihilation cross section\, testing new\nanalysis tools for the investigation of extended regions. In this talk\, I\nwill present both results achieved by MAGIC and the importance of DM\ntailored analysis tools and the proper selection of new dSph targets\, in\norder to propose scientific cases for CTA\, the upcoming generation of\nCherenkov telescopes.
URL:https://www.oa-roma.inaf.it/event/talk-by-paola-giammaria/
LOCATION:RM
CATEGORIES:Seminari
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BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20170606T114500
DTEND;TZID=Europe/Rome:20170606T124500
DTSTAMP:20260405T142254
CREATED:20170412T103150Z
LAST-MODIFIED:20170412T103150Z
UID:4709-1496749500-1496753100@www.oa-roma.inaf.it
SUMMARY:Dwarf spheroidal satellite galaxies under the eye of Cherenkov telescopes: indirect search for dark matter by MAGIC and opportunities and prospects for CTA
DESCRIPTION:Searching for gamma-ray signals from dark matter annihilation in dwarf\nspheroidal satellite galaxies (dSphs) of the Milky Way plays a critical\nrole within the framework of indirect dark matter searches. This study\,\naimed at unveiling the nature of the most elusive component of the\nUniverse\, is potentially able to confirm the dark matter interpretation of\nthe observed gamma-ray excess in the Galactic Center.\nThanks to deep observation campaigns on dSphs\, MAGIC achieved stringent\nconstraints to dark matter annihilation cross section\, testing new\nanalysis tools for the investigation of extended regions. In this talk\, I\nwill present both results achieved by MAGIC and the importance of DM\ntailored analysis tools and the proper selection of new dSph targets\, in\norder to propose scientific cases for CTA\, the upcoming generation of\nCherenkov telescopes.
URL:https://www.oa-roma.inaf.it/event/talk-by-paola-giammaria-2/
LOCATION:RM
CATEGORIES:Seminari
END:VEVENT
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