BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//CERN//INDICO//EN
BEGIN:VEVENT
SUMMARY:Search for a Dark Matter annihilation signal from the Sagittarius 
 dwarf galaxy with H.E.S.S.
DTSTART;VALUE=DATE-TIME:20070710T143000Z
DTEND;VALUE=DATE-TIME:20070710T144200Z
DTSTAMP;VALUE=DATE-TIME:20261017T114654Z
UID:indico-contribution-496@cern.ch
DESCRIPTION:Speakers: Dr. MOULIN\, Emmanuel (DAPNIA/SPP)\nDwarf Sphreroida
 l galaxies are amongst the best target to search for a Dark Matter\nannihi
 lation signal. The annihilation of WIMPs in the center of Sgr dwarf would\
 nproduce high energy gamma-rays in the final state. Observations carried o
 ut with the\nH.E.S.S. array of Imaging Atmospheric Cherenkov telescopes ar
 e presented. A careful\nmodelling of the Dark Matter halo profile of Sgr d
 warf was performed using latest\nmeasurements on its structural parameters
 . Constraints on the velocity-weighted cross\nsection of Dark Matter parti
 cles are derived in the framework of Supersymmetric and\nKaluza-Klein mode
 ls.\n\nhttps://indico.nucleares.unam.mx/event/4/session/65/contribution/49
 6
LOCATION:Merida\, Mexico Kabah (Holiday Inn)
URL:https://indico.nucleares.unam.mx/event/4/session/65/contribution/496
END:VEVENT
END:VCALENDAR