about
Observation of tau neutrino appearance in the CNGS beam with the OPERA experimentSearch for Magnetic Monopoles with the MoEDAL Forward Trapping Detector in 13 TeV Proton-Proton Collisions at the LHC.Discovery of τ Neutrino Appearance in the CNGS Neutrino Beam with the OPERA Experiment.Observation of a first ν τ candidate event in the OPERA experiment in the CNGS beamMeasurement of the neutrino velocity with the OPERA detector in the CNGS beamSearch for magnetic monopoles with the MoEDAL forward trapping detector in 2.11 fb −1 of 13 TeV proton–proton collisions at the LHCFinal Results of the OPERA Experiment on ν_{τ} Appearance in the CNGS Neutrino BeamMomentum measurement by the multiple Coulomb scattering method in the OPERA lead-emulsion targetSearch forνμ→ντoscillation with the OPERA experiment in the CNGS beamStudy of neutrino interactions with the electronic detectors of the OPERA experimentMeasurement of the atmospheric muon charge ratio with the OPERA detectorThe OPERA experiment in the CERN to Gran Sasso neutrino beamPlanck intermediate results LI. Features in the cosmic microwave background temperature power spectrum and shifts in cosmological parametersPlanck intermediate results XLVI. Reduction of large-scale systematic effects in HFI polarization maps and estimation of the reionization optical depthPlanck intermediate results LII. Planet flux densitiesPlanck intermediate results L. Evidence of spatial variation of the polarized thermal dust spectral energy distribution and implications for CMB B-mode analysisPlanck intermediate results XLIV. Structure of the Galactic magnetic field from dust polarization maps of the southern Galactic capPlanck intermediate results XLIX. Parity-violation constraints from polarization dataPlanck intermediate results XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropiesMeasurement of low-energy neutrino cross-sections with the PEANUT experimentStudy of the effects induced by lead on the emulsion films of the OPERA experimentSearch for magnetic monopoles with the MoEDAL prototype trapping detector in 8 TeV proton-proton collisions at the LHCThe physics programme of the MoEDAL experiment at the LHCAn integrated system for large scale scanning of nuclear emulsionsImproving the detection efficiency in nuclear emulsion trackersErratum: new results on ν μ → ν τ appearance with the OPERA experiment in the CNGS beamEvidence forνμ→ντappearance in the CNGS neutrino beam with the OPERA experimentMeasurement of the TeV atmospheric muon charge ratio with the complete OPERA data setProcedure for short-lived particle detection in the OPERA experiment and its application to charm decaysA fast automatic plate changer for the analysis of nuclear emulsionsAddendum: search for ν μ → ν e oscillations with the OPERA experiment in the CNGS beamMeasurement of the neutrino velocity with the OPERA detector in the CNGS beam using the 2012 dedicated dataNew results on ν μ → ν τ appearance with the OPERA experiment in the CNGS beamSearch for ν μ → ν e oscillations with the OPERA experiment in the CNGS beamDetermination of a time-shift in the OPERA set-up using high-energy horizontal muons in the LVD and OPERA detectorsSearch for sterile neutrinos in muon neutrino disappearance mode at FNALDetailed design and first tests of the application software for the instrument control unit of Euclid-NISPEuclid Near Infrared Spectrometer and Photometer instrument concept and first test results obtained for different breadboards models at the end of phase CEmulsion sheet doublets as interface trackers for the OPERA experimentDetermination of the muon charge sign with the dipolar spectrometers of the OPERA experiment
P50
Q27019912-73219345-408B-4473-9BCD-DFFBA6496F49Q50874454-853BDDE5-B8A2-4CD1-9AA9-CFC3B8E4FE9BQ53192805-089D4EB3-FA6E-4854-9027-4E4250EC8147Q55897636-6B469D94-B742-4B84-ABAE-329E0D2A3C9CQ55897674-F4CEDA74-CF98-4745-8088-C8BDB7E90212Q55950516-71EAF9F9-503D-4B89-9BA2-51CFFCEE87FAQ56381152-A6A04036-4A51-49A1-A4DE-2EC8D343C045Q57598507-0EB6DEBD-4BD9-4273-BF61-6ACFDD690D3BQ57598508-610C3D86-4C7C-4CD2-B422-8C4B2782860CQ57598509-60F74D14-DB5C-45DD-88A6-17209FEB5733Q57598512-D5086C29-6D74-4A3B-8124-E5EE9B450034Q57598517-A1CD7E8E-76E9-4912-821E-2CE761854E20Q57630580-2D960380-006E-46DB-AFC2-FDD74A8511A5Q57630580-37BB3498-6659-43FE-96F4-EE810AFAE730Q57630604-32547C43-6DC6-41E7-B3FF-D68416677D09Q57630604-8AA906AE-83BE-471C-BBCA-964D0286A50AQ57633574-6E4A3BDF-3305-4F9D-9B06-DCF1EABFCC42Q57633574-D0FFFB05-FBE8-4C80-9A7F-4B670EE2E602Q57633581-3FFC045A-1513-4DC6-A77A-7A12D3CDC746Q57633581-D8B4BC66-1F98-484E-B175-9F425605DCE5Q57633591-0AE2284D-A309-43A2-BE8A-78CCF4F13F37Q57633592-23076784-27E0-43CB-B1BA-51C4AFBC3871Q57633592-EAA92E2D-3FDA-49A8-8B45-0CE50F37CCA0Q57633596-36CBC99F-873F-4A3A-BF29-BE55A8695F74Q57633596-39F31B0C-361F-4C18-AD2D-7F758250D250Q57714844-C5B33DA8-26A2-4F40-8163-D3D1A7E47D0CQ57714856-1FCECBCB-DE29-4E6D-9B40-C9D3A31CEFD4Q57722915-6A8DB997-54A6-4652-8ACC-1D28F02C93B1Q57722926-E812E7E8-9991-49FA-A6E6-6B1B49E0DB84Q57910363-87AFD4C4-9B4C-41F2-AB28-68D72E498013Q58335613-96F53659-E0E3-4B2D-8CF3-2C67C88BAD9BQ58335615-4851DB74-922E-4193-A79E-157A235DF07DQ58335616-8C46A371-D13E-4E81-85A6-7705A731C7DCQ58335617-6869378C-616D-44A6-9462-3B3F65E7FA05Q58335618-FE5B0059-0AD9-43AD-98D2-94898CFD5B9DQ58335619-8EC71400-2485-4AE3-98D4-C693984AB990Q58335620-22452BD5-94DD-46EC-858A-6CFA09518ADCQ58335621-083A2C3C-1CAD-4BA2-88F1-79BA72B6D09BQ58335622-E22B3492-BF4B-4FEA-8872-03D6988B917EQ58335623-886EB71F-F5A8-4ED6-9E11-C206C17759C9
P50
description
researcher
@en
wetenschapper
@nl
հետազոտող
@hy
name
M Tenti
@nl
Matteo Tenti
@en
Matteo Tenti
@es
type
label
M Tenti
@nl
Matteo Tenti
@en
Matteo Tenti
@es
altLabel
M Tenti
@en
prefLabel
M Tenti
@nl
Matteo Tenti
@en
Matteo Tenti
@es
P106
P1153
35194662000
P21
P31
P496
0000-0002-4254-5901