Speaker
Mr
Stefan Coenders
(Technische Universität München)
Description
The IceCube Neutrino Observatory located at the geographic South Pole was designed
to study and discover high energy neutrinos coming from both galactic and
extragalactic astrophysical sources. Track-like events induced by charged-current
muon-neutrino interactions close to the IceCube detector give an angular resolution
better than 1° above TeV energies.
We present here the results of searches for pointlike astrophysical neutrino sources
on the full sky using 6 years of detector livetime, of which three years use the complete IceCube detector.
Within 2000 days of detector livetime, IceCube is sensitive to a steady flux substantially below
$E^2\,\partial\phi\,/\,\partial E=10^{-12}\mathrm{TeV\,cm^{-2}\,s^{-1}}$ in the northern
hemisphere for neutrino energies above 10~TeV.
Author
Mr
Stefan Coenders
(Technische Universität München)
