about
Dark Matter Results from 100 Live Days of XENON100 DataThe neutron background of the XENON100 dark matter search experimentObservation and applications of single-electron charge signals in the XENON100 experimentImplications on inelastic dark matter from 100 live days of XENON100 dataMeasurement of the Velocity of Neutrinos from the CNGS Beam with the Large Volume DetectorDark Matter Results from 225 Live Days of XENON100 DataFirst Dark Matter Search Results from the XENON1T Experiment.Limits on spin-dependent WIMP-nucleon cross sections from 225 live days of XENON100 data.Analysis of the XENON100 dark matter search dataResponse of the XENON100 dark matter detector to nuclear recoilsThe distributed Slow Control System of the XENON100 experimentPerformances and stability of a 2.4 ton Gd organic liquid scintillator target for ν̄edetectionFirst CNGS events detected by LVDStudy of the effect of neutrino oscillations on the supernova neutrino signal in the LVD detectorCNGS beam monitor with the LVD detectorStudy of the effect of neutrino oscillation on the supernova neutrino signal with the LVD detectorCNGS beam monitor with the LVD detectorSearch for low energy ν in correlation with the 8 events observed by the EXPLORER and NAUTILUS detectors in 2001Study of single muons with the Large Volume Detector at the Gran Sasso LaboratoryStudy of the c.r. composition and interaction at E0 = 10 – 100 TeV from the observation of H.E. muons and atmospheric Cherenkov light in EASThe high energy muon spectrum in Extensive Air Showers: first data from LVD and EAS-TOP at Gran SassoDetermination of a time-shift in the OPERA set-up using high-energy horizontal muons in the LVD and OPERA detectorsThe EEE Project: cosmic rays, multigap resistive plate chambers and high school studentsObservation of the February 2011 Forbush decrease by the EEE telescopesInternational Scoping Study (ISS) for a future neutrino factory and Super-Beam facility. Detectors and flux instrumentation for future neutrino facilitiesFirst detection of extensive air shower with the EEE experimentTowards the installation and use of an extended array for cosmic ray detection: The EEE ProjectExtreme Energy Events Project: Construction of the detectors and installation in Italian High SchoolsPerformance of a six gap MRPC built for large area coverageEEE project: Science in the schoolsMultigap resistive plate chambers for EAS study in the EEE ProjectThe EEE Project: status and perspectivesDetermining the hierarchy of neutrino masses with high density magnetized detectors at the Beta BeamsNeutrino hierarchy from CP-blind observables with high density magnetized detectorsMaterial radioassay and selection for the XENON1T dark matter experimentUpper limit on the prompt muon flux derived from the LVD underground experimentMuon “depth-intensity” relation measured by the LVD underground experiment and cosmic-ray muon spectrum at sea level
P50
Q21563731-1B183B39-7882-432F-84F6-C7903D082486Q27015368-206DABE0-D989-4645-BA3A-1DE961638F43Q27016688-B6729BF6-5DA4-4E43-92C0-1B415DC388CEQ27444453-669B61F4-C227-4444-AC6B-D20762646F73Q27448848-F99CC404-0566-4404-964A-6BB419619D19Q27449454-50744EC8-0CE0-4EE7-9EF2-F454E8BC2C03Q50011013-6FAC295F-7BBD-40A5-8C80-5D69E40B1750Q55057285-039348C0-C932-47C0-A798-B5ECF02821D2Q58314854-15335C5E-46ED-4DEF-A3EC-EEC4AA887C5CQ58314861-19665DF2-52B4-4310-886C-EAA71995AE99Q58314866-C839BA22-F9DD-4F09-98B1-00702B3165D5Q58314874-B1D3DC31-0DBB-4D11-BCDA-4E044C71F6B1Q58314894-734BA0FD-0CFF-48F2-B9EA-488499FC2454Q58314895-9C549BBA-5F43-4F54-812F-4A324407937AQ58314897-8C0CC464-2D51-4480-A8E6-F6F5D304BEFBQ58314899-CEC1CF2B-9E1C-48B8-821E-5C2C12DB68F1Q58314900-645B469D-EDDA-4476-A3CE-AA10A8895B27Q58314902-A661821A-B919-4D90-B5B4-4D38E8164846Q58314918-16C4067B-4DB4-4BCE-90EB-C239BDC657E0Q58317104-C91E4509-4564-4A02-9795-2D73D82654B6Q58317105-3BDBA5D3-5A15-4E68-AE37-7677A892E062Q58335624-5A74D992-62B0-4E5F-908F-9C3121B8FAD9Q58357732-96F664E4-7AA7-43C9-8D8A-1D832B8B65BBQ58357735-34A9A102-6364-4480-8A0B-EED78FADA56AQ58361312-B3A95E4D-60EA-4E63-BDD7-15DBD3A070C0Q58379090-6B87F755-D4DC-4AAF-865C-E0E73E94E993Q58379098-430D37CE-E02B-44EE-BBF8-5381D7723E47Q58379103-3FF730CB-776D-4706-A261-6AFE79EC53A2Q58379106-EF3303A5-70C3-4043-B17E-F1ED8891FB40Q58379112-736A9C25-7A1D-40D9-B7D4-08FB4C26BD17Q58379116-4D003BEB-89E1-4BDA-9831-912278FD432DQ58379122-836E6ECD-6F1A-4D16-A4CF-26018E4D4999Q58382738-346B0E20-A0DE-434B-9905-3EA12C83C73CQ58382741-BAE5E416-AD89-44B3-947D-F3F20588B052Q58808468-2E19ADF2-D2D5-412F-A4D9-8B3A9F81BCEEQ59660994-D72D7C4D-9C0E-4701-826C-07FE3A245BB2Q59660995-BF5E5D74-E4A0-472B-9C82-B75AB0D7D9E8
P50
description
researcher
@en
wetenschapper
@nl
հետազոտող
@hy
name
Marco Selvi
@ast
Marco Selvi
@br
Marco Selvi
@co
Marco Selvi
@cs
Marco Selvi
@da
Marco Selvi
@de
Marco Selvi
@en
Marco Selvi
@es
Marco Selvi
@fr
Marco Selvi
@id
type
label
Marco Selvi
@ast
Marco Selvi
@br
Marco Selvi
@co
Marco Selvi
@cs
Marco Selvi
@da
Marco Selvi
@de
Marco Selvi
@en
Marco Selvi
@es
Marco Selvi
@fr
Marco Selvi
@id
prefLabel
Marco Selvi
@ast
Marco Selvi
@br
Marco Selvi
@co
Marco Selvi
@cs
Marco Selvi
@da
Marco Selvi
@de
Marco Selvi
@en
Marco Selvi
@es
Marco Selvi
@fr
Marco Selvi
@id
P106
P1153
6603935386
P31
P496
0000-0003-0243-0840