Capability of the HAWC Gamma-Ray Observatory for the Indirect Detection of Ultrahigh-Energy Neutrinos

Advances in Astronomy - United States
doi 10.1155/2017/1932413
Full Text
Abstract

Available in full text

Date
Authors
Publisher

Hindawi Limited

Related search

Upgrade Paths for the HAWC Gamma-Ray Observatory

2016English

Gamma-Ray Astronomy With the Hawc Observatory

International Journal of Modern Physics: Conference Series
2014English

On the Detection of Ultra High Energy Neutrinos With the Auger Observatory

Astroparticle Physics
AstrophysicsAstronomy
1998English

Multiple Gamma-Ray Detection Capability of a CeBr3 Detector for Gamma Spectroscopy

Journal of Spectroscopy
OpticsAnalytical ChemistryAtomicSpectroscopyMolecular Physics,
2017English

Information Technologies on High-Energy Astrophysics: Cosmic Ray Anisotropy Using HAWC Observatory

EPJ Web of Conferences
AstronomyPhysics
2019English

Sensitivity of HAWC to Gamma Ray Bursts

2012English

Time-Dependent Search for Neutrino Emission From MRK 421 and MRK 501 Observed by the HAWC Gamma-Ray Observatory

2017English

Detectability of Ultrahigh Energy Cosmic-Ray Signatures in Gamma-Rays

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2011English

The New Gamma Ray Telescope Observatory: CTA

2016English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2025 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy