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SUMMARY:Search for gamma-ray emission from Unidentified EGRET sources Loca
 ted in the Cygnus Region with the MAGIC Telescope
DTSTART;VALUE=DATE-TIME:20070704T153000Z
DTEND;VALUE=DATE-TIME:20070704T154200Z
DTSTAMP;VALUE=DATE-TIME:20260717T180308Z
UID:indico-contribution-484@cern.ch
DESCRIPTION:Speakers: Mr. BARTKO\, Hendrik (MPI f. Physik\, Munich\, Germa
 ny)\nMany of the unidentified Egret sources are believed to be young pulsa
 rs.\nSuch young not-identified pulsars should be surrounded by pulsar wind
 \nnebulae which are at present well established TeV gamma-ray sources\n(li
 ke Vela X\, MSH 15-52 and G0.9+0.1). Moreover\, other type of\ngamma-ray s
 ources are likely\, i.e. binary systems\, molecular clouds\,\nsupernovae\n
 remnants\, massive stars. The Milagro experiment has recently reported\na 
 gamma-ray source above ~12 TeV in the Cygnus region\, MGRO J2019+37\,\nwhi
 ch is spatially coincident with the EGRET sources 3EG J2021+3716 /\n3EG J2
 016+3657.\nHere we present the results of a search for gamma-ray emission 
 between about\n100 GeV and about 10 TeV with the MAGIC telescope from thes
 e sources.\n\nhttps://indico.nucleares.unam.mx/event/4/session/103/contrib
 ution/484
LOCATION:Merida\, Mexico Uxmal + Tulum (Holiday Inn)
URL:https://indico.nucleares.unam.mx/event/4/session/103/contribution/484
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