PoS - Proceedings of Science
Volume 283 - Neutrino Oscillation Workshop (NOW2016) - Session III: Multimessanger astrophysics
Ultra-high energy multi-messengers at the Pierre Auger Observatory
J. Alvarez-Muniz* on behalf of the Pierre Auger Collaboration
*corresponding author
Full text: pdf
Pre-published on: March 05, 2017
Published on: June 20, 2017
The Pierre Auger Observatory is the largest ultra-high
energy cosmic-ray detector in the world. With the Surface
Detector array of the Observatory we can also search
for neutral particles that point back to their sources
of production. In particular, ultra-high energy neutrinos
and photons, with energies around 1 EeV and above,
can be identified, and the most stringent limits at EeV energies
are set to their fluxes from a large fraction of the sky. These
limits provide additional information on the nature of the
ultra-high energy cosmic rays which may help identifying
the sources where they are accelerated up to 100 EeV.
DOI: https://doi.org/10.22323/1.283.0056
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.

Open Access
Creative Commons LicenseCopyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.