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SUMMARY:VHE gamma-ray observations of the pulsar PSR B1951+32 and its asso
 ciated nebula CTB 80 with the MAGIC Telescope.
DTSTART;VALUE=DATE-TIME:20070704T175300Z
DTEND;VALUE=DATE-TIME:20070704T180500Z
DTSTAMP;VALUE=DATE-TIME:20260819T200956Z
UID:indico-contribution-1023@cern.ch
DESCRIPTION:Speakers: Ms. DE LOS REYES\, Raquel (Complutense University of
  Madrid)\, Ms. ALIU\, Ester (Institut de Fisica d'Altes Energies)\nObserva
 tions of pulsars and pulsar wind nebulae \nhave been conducted during the 
 last two years using the \nMAGIC Imaging Cerenkov Telescope. In addition t
 o the study\nof the nebula emission\, the low energy threshold of MAGIC\no
 ffers the opportunity to search for the pulsed emission\nwith very high se
 nsitivity.\nThe selection of the objects was based on their spin-down lumi
 nosity \nand the probability of emission given the various models of VHE \
 n$\\gamma$-ray production above 100 GeV. \n\nWe present the results of the
 se observations and their implication\nfor models of VHE emission.\n\nhttp
 s://indico.nucleares.unam.mx/event/4/session/5/contribution/1023
LOCATION:Merida\, Mexico Uxmal + Tulum (Holiday Inn)
URL:https://indico.nucleares.unam.mx/event/4/session/5/contribution/1023
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