Search for PeV Gamma-Ray Point Sources with IceCube
Z. Griffith*, H. Pandya on behalf of the IceCube Collaboration
August 16, 2017
August 03, 2018
We present results of a search for PeV gamma-ray point sources with the IceCube Neutrino Observatory, presently the most sensitive facility for PeV gamma-ray sources in the southern hemisphere. This includes a general search over IceCube’s field of view, as well as tests for correlations with TeV sources detected by H.E.S.S. and neutrino events from IceCube’s high-energy starting event sample. As the attenuation length of PeV gamma rays limits observational distances to within the Galaxy, one of the goals of the analysis is to constrain the Galactic component of the astrophysical neutrino flux observed by IceCube.
How to cite
Metadata are provided both in "article" format (very similar to INSPIRE) as this helps creating
very compact bibliographies which can be beneficial to authors and
readers, and in "proceeding" format
which is more detailed and complete.