Add to ORKGMACRO experiment operated in the Gran Sasso underground laboratory. Neutrino events collected by this detector are used in order to study the atmospheric neutrino flux. Different measurements in different energy samples are in full agreement and show evidence of neutrino oscillation phenomenon. Also the search for neutrino astrophysical sources is reported
AbstractThe energy of atmospheric neutrinos detected by MACRO was estimated using multiple Coulomb s...
A large area underground detector with accurate muon tracking and directionality can be used for the...
High energy neutrinos from astrophysical sources can be detected as upward-going muons produced in c...
After a brief presentation of the MACRO detector we discuss the updated data on atmospheric muon neu...
The results of the MACRO experiment on atmospheric neutrino oscillations are presented and discussed...
In this paper we first give a short overview of the MACRO detector, which was operational at the Gra...
After a short overview of the MACRO detector, located at the Gran Sasso Laboratory, I shall present ...
After a brief presentation of the MACRO detector we discuss the data on atmospheric neutrinos and ne...
MACRO can detect three topologies of neutrino induced events, corresponding to different parent neut...
The events collected with the lower part of the MACRO detector at the Gran Sasso Laboratory have bee...
A measurement of the flux of neutrino-induced muons using the MACRO detector is presented. Different...
In this paper I shall resume the results of the MACRO experiment on atmospheric muon neutrino oscill...
The results of the MACRO experiment on atmospheric neutrino oscillations are presented and discussed...
The results of the MACRO experiment on atmospheric neutrino oscillations are presented and discussed...
We discuss the final results of the MACRO experiment on atmospheric neutrino oscillations. The data ...
AbstractThe energy of atmospheric neutrinos detected by MACRO was estimated using multiple Coulomb s...
A large area underground detector with accurate muon tracking and directionality can be used for the...
High energy neutrinos from astrophysical sources can be detected as upward-going muons produced in c...
After a brief presentation of the MACRO detector we discuss the updated data on atmospheric muon neu...
The results of the MACRO experiment on atmospheric neutrino oscillations are presented and discussed...
In this paper we first give a short overview of the MACRO detector, which was operational at the Gra...
After a short overview of the MACRO detector, located at the Gran Sasso Laboratory, I shall present ...
After a brief presentation of the MACRO detector we discuss the data on atmospheric neutrinos and ne...
MACRO can detect three topologies of neutrino induced events, corresponding to different parent neut...
The events collected with the lower part of the MACRO detector at the Gran Sasso Laboratory have bee...
A measurement of the flux of neutrino-induced muons using the MACRO detector is presented. Different...
In this paper I shall resume the results of the MACRO experiment on atmospheric muon neutrino oscill...
The results of the MACRO experiment on atmospheric neutrino oscillations are presented and discussed...
The results of the MACRO experiment on atmospheric neutrino oscillations are presented and discussed...
We discuss the final results of the MACRO experiment on atmospheric neutrino oscillations. The data ...
AbstractThe energy of atmospheric neutrinos detected by MACRO was estimated using multiple Coulomb s...
A large area underground detector with accurate muon tracking and directionality can be used for the...
High energy neutrinos from astrophysical sources can be detected as upward-going muons produced in c...