about
Description of atmospheric conditions at the Pierre Auger Observatory using the Global Data Assimilation System (GDAS)Search for signatures of magnetically-induced alignment in the arrival directions measured by the Pierre Auger ObservatoryThe Lateral Trigger Probability function for the Ultra-High Energy Cosmic Ray showers detected by the Pierre Auger ObservatoryUpper limit on the cosmic-ray photon fraction at EeV energies from the Pierre Auger ObservatoryFinal results of Borexino Phase-I on low-energy solar neutrino spectroscopySEARCHES FOR LARGE-SCALE ANISOTROPY IN THE ARRIVAL DIRECTIONS OF COSMIC RAYS DETECTED ABOVE ENERGY OF 10 19 eV AT THE PIERRE AUGER OBSERVATORY AND THE TELESCOPE ARRAYNeutrino physics with JUNOThe fluorescence detector of the Pierre Auger ObservatoryPrecision measurement of the (7)Be solar neutrino interaction rate in BorexinoNew limits on heavy sterile neutrino mixing in B 8 decay obtained with the Borexino detectorDirect Measurement of the Be 7 Solar Neutrino Flux with 192 Days of Borexino DataFirst Evidence of p e p Solar Neutrinos by Direct Detection in BorexinoSearch for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory.Lifetimes of (214)Po and (212)Po measured with Counting Test Facility at Gran Sasso National Laboratory.Testing Hadronic Interactions at Ultrahigh Energies with Air Showers Measured by the Pierre Auger Observatory.Measurement of the Radiation Energy in the Radio Signal of Extensive Air Showers as a Universal Estimator of Cosmic-Ray Energy.Test of Electric Charge Conservation with Borexino.Search for electron decay mode e→γ+ν with prototype of Borexino detectorCombined fit of spectrum and composition data as measured by the Pierre Auger ObservatorySpectral calibration of the fluorescence telescopes of the Pierre Auger ObservatoryAn Indication of Anisotropy in Arrival Directions of Ultra-high-energy Cosmic Rays through Comparison to the Flux Pattern of Extragalactic Gamma-Ray SourcesMeasurement of the energy spectrum of cosmic rays above 1018 eV using the Pierre Auger ObservatorySpectroscopy of geoneutrinos from 2056 days of Borexino dataSearch for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger ObservatoryBorexino’s search for low-energy neutrino and antineutrino signals correlated with gamma-ray burstsSeasonal modulation of the 7 Be solar neutrino rate in BorexinoHigh significance measurement of the terrestrial neutrino flux with the Borexino detectorRecent results from BorexinoSOX: search for short baseline neutrino oscillations with BorexinoRecent results from Borexino and the first real time measure of solar pp neutrinosCNO andpepsolar neutrino measurements and perspectives in BorexinoGeo-neutrino results with BorexinoMeasurement of Solar pp-neutrino flux with Borexino: results and implicationsOverview and accomplishments of the Borexino experimentTest of the electric charge conservation law with Borexino detectorThe144Ce source for SOXThe high precision measurement of the144Ce activity in the SOX experimentUnderstanding the detector behavior through Montecarlo and calibration studies in view of the SOX measurementFirst real–time detection of solar pp neutrinos by BorexinoShort distance neutrino oscillations with Borexino
P50
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P50
description
onderzoeker
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researcher
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հետազոտող
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Lino Miramonti
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Lino Miramonti
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Lino Miramonti
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Lino Miramonti
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@id
P214
P244
P1053
J-3217-2012
P106
P1153
57196834655
6701399152
P21
P214
P244
no2014001428
P31
P496
0000-0002-2808-5363
P7859
lccn-no2014001428