Add to ORKGA search for diffuse neutrinos with energies in excess of 105 GeV is conducted with AMANDA-II data recorded between 2000 and 2002. Above 107 GeV, the Earth is essentially opaque to neutrinos. This fact, combined with the limited overburden of the AMANDA-II detector (roughly 1.5 km), concentrates these ultra high-energy neutrinos at the horizon. The primary background for this analysis is bundles of downgoing, high-energy muons from the interaction of cosmic rays in the atmosphere. No statistically significant excess above the expected background is seen in the data, and an upper limit is set on the diffuse all-flavor neutrino flux of E2 90%CL <2.7 × 10−7 GeV cm−2 s−1 sr−1 valid over the energy range of 2 × 105 GeV to 109 GeV. A number of mo...
Interactions of cosmic rays with the galactic interstellar medium produce high-energy neutrinos thro...
The results of a search for point sources of high energy neutrinos in the northern hemisphere using ...
We present a search for point sources of high energy neutrinos using 3.8 yr of data recorded by AMAN...
A search for diffuse neutrinos with energies in excess of 105 GeV is conducted with AMANDA-II data r...
A search for diffuse neutrinos with energies in excess of 105 GeV is conducted with AMANDA-II data r...
A search for diffuse neutrinos with energies in excess of 105 GeV is conducted with AMANDA-II data r...
A search for diffuse neutrinos with energies in excess of 10⁵ GeV is conducted with AMANDA-II data r...
A search for a diffuse flux of cosmic neutrinos with energies in excess of 1014 eV was performed usi...
High-energy neutrinos are capable of carrying information over vast distances, and neutrino telescop...
A search for TeV-PeV muon neutrinos from unresolved sources was performed on AMANDA-II data collecte...
We report on a search for electro-magnetic and/or hadronic showers (cascades) induced by high-energy...
We report on a search for electro-magnetic and/or hadronic showers (cascades) induced by high energy...
We describe the search for astrophysical sources of high energy neutrinos with the AMANDA-II detecto...
Data taken during 1997 with the AMANDA-B10 detector are searched for a diffuse flux of neutrinos of ...
Many galactic and extragalactic astrophysical sources are currently considered promising candidates ...
Interactions of cosmic rays with the galactic interstellar medium produce high-energy neutrinos thro...
The results of a search for point sources of high energy neutrinos in the northern hemisphere using ...
We present a search for point sources of high energy neutrinos using 3.8 yr of data recorded by AMAN...
A search for diffuse neutrinos with energies in excess of 105 GeV is conducted with AMANDA-II data r...
A search for diffuse neutrinos with energies in excess of 105 GeV is conducted with AMANDA-II data r...
A search for diffuse neutrinos with energies in excess of 105 GeV is conducted with AMANDA-II data r...
A search for diffuse neutrinos with energies in excess of 10⁵ GeV is conducted with AMANDA-II data r...
A search for a diffuse flux of cosmic neutrinos with energies in excess of 1014 eV was performed usi...
High-energy neutrinos are capable of carrying information over vast distances, and neutrino telescop...
A search for TeV-PeV muon neutrinos from unresolved sources was performed on AMANDA-II data collecte...
We report on a search for electro-magnetic and/or hadronic showers (cascades) induced by high-energy...
We report on a search for electro-magnetic and/or hadronic showers (cascades) induced by high energy...
We describe the search for astrophysical sources of high energy neutrinos with the AMANDA-II detecto...
Data taken during 1997 with the AMANDA-B10 detector are searched for a diffuse flux of neutrinos of ...
Many galactic and extragalactic astrophysical sources are currently considered promising candidates ...
Interactions of cosmic rays with the galactic interstellar medium produce high-energy neutrinos thro...
The results of a search for point sources of high energy neutrinos in the northern hemisphere using ...
We present a search for point sources of high energy neutrinos using 3.8 yr of data recorded by AMAN...