Add to ORKGThe shadowing of high-energy cosmic rays by the Moon has been observed with a significance of 9.4 standard deviations with the L3 + C muon spectrometer at CERN. A significant effect of the Earth magnetic field is observed. Since no event deficit on the east side of the Moon has been observed, an upper limit at 90% confidence level on the antiproton to proton ratio of 0.11 is obtained for primary energies around 1 TeV.Facultad de Ciencias Exacta
Data collected by the Pierre Auger Observatory provide evidence for anisotropy in the arrival direct...
The energy spectrum of cosmic rays above 2.5 x 1018 eV, derived from 20 000 events recorded at the P...
A precision measurement by AMS of the positron fraction in primary cosmic rays in the energy range f...
The shadowing of high-energy cosmic rays by the Moon has been observed with a significance of 9.4 st...
The Astrophysical Journal 758.2 (2012): 140 reproduced by permission of the AASWe report on the dete...
The L3+C muon detector at the CERN electron–positron collider, LEP, is used for the detection of ver...
We report on the detection of high-energy -ray emission from the Moon during the first 24 months of...
We report on the observation of a significant deficit of cosmic rays from the direction of the Moon ...
One of the main objectives of the ANTARES telescope is the search for point-like neutrino sources. B...
This article reports the first observation of the Moon and the Sun shadows in the sky distribution o...
The energy spectrum of cosmic rays above 2.5×1018eV, derived from 20000 events recorded at the Pierr...
Data collected by the Pierre Auger Observatory through 31 August 2007 showed evidence for anisotropy...
An indirect measurement of the antiproton flux in cosmic rays is possible as the particles undergo d...
The energy spectrum of cosmic rays above 2.5x10^18eV, derived from 20,000 events recorded at the Pie...
We have measured the gamma-ray emission spectrum of the Moon using the data collected by the Large A...
Data collected by the Pierre Auger Observatory provide evidence for anisotropy in the arrival direct...
The energy spectrum of cosmic rays above 2.5 x 1018 eV, derived from 20 000 events recorded at the P...
A precision measurement by AMS of the positron fraction in primary cosmic rays in the energy range f...
The shadowing of high-energy cosmic rays by the Moon has been observed with a significance of 9.4 st...
The Astrophysical Journal 758.2 (2012): 140 reproduced by permission of the AASWe report on the dete...
The L3+C muon detector at the CERN electron–positron collider, LEP, is used for the detection of ver...
We report on the detection of high-energy -ray emission from the Moon during the first 24 months of...
We report on the observation of a significant deficit of cosmic rays from the direction of the Moon ...
One of the main objectives of the ANTARES telescope is the search for point-like neutrino sources. B...
This article reports the first observation of the Moon and the Sun shadows in the sky distribution o...
The energy spectrum of cosmic rays above 2.5×1018eV, derived from 20000 events recorded at the Pierr...
Data collected by the Pierre Auger Observatory through 31 August 2007 showed evidence for anisotropy...
An indirect measurement of the antiproton flux in cosmic rays is possible as the particles undergo d...
The energy spectrum of cosmic rays above 2.5x10^18eV, derived from 20,000 events recorded at the Pie...
We have measured the gamma-ray emission spectrum of the Moon using the data collected by the Large A...
Data collected by the Pierre Auger Observatory provide evidence for anisotropy in the arrival direct...
The energy spectrum of cosmic rays above 2.5 x 1018 eV, derived from 20 000 events recorded at the P...
A precision measurement by AMS of the positron fraction in primary cosmic rays in the energy range f...