Search for Neutrinos from Strong Variable Gamma Ray Sources. Wolfgang Rhode Dortmund. Challenge. 5 years of data taken with AMANDA Up to now: no extraterrestric signal found most interesting hint: from coincidence analysis with HEGRA. The Sky in TeV-Light 2003. ~ 5 variable sources
Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author.While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server.
Search for Neutrinos from Strong Variable Gamma Ray Sources
~ 5 variable sources
at the nothern hemisphere
This plot could have
been made by telescopes
of a sensitivity of 1 single
1 < g/n < 50 (KM)
3 years of IceCube
Fig1: Whipple data, Eth=600 GeV 
Fig2: HEGRA data, Eth=1 TeV 
From the analysis of 1ES1959+650 we have learned, that by coincident observations a singificant background (time) reduction (factor 10-100) becomes possible.
will be done