about
The CMS experiment at the CERN LHCDescription 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 ObservatoryThe fluorescence detector of the Pierre Auger ObservatoryObservation of the Suppression of the Flux of Cosmic Rays above 4 × 10 19 eVCorrelation of the highest-energy cosmic rays with nearby extragalactic objects.Measurement of the energy spectrum of cosmic rays above 1018 eV using the Pierre Auger ObservatoryA targeted search for point sources of EeV neutronsA search for point sources of EeV photonsSearch for heavy neutral lepton production in K + decaysThe beam and detector of the NA62 experiment at CERNAn upper limit to the photon fraction in cosmic rays above 1019eV from the Pierre Auger ObservatoryAnisotropy studies around the galactic centre at EeV energies with the Auger ObservatoryReconstruction of the signal amplitude of the CMS electromagnetic calorimeterResults of the first performance tests * of the CMS electromagnetic calorimeterUltrahigh Energy Neutrinos at the Pierre Auger ObservatoryConstraints on the origin of cosmic rays above 10^18^ eV from large-scale anisotropy searches in data of the pierre auger observatoryA search for point sources of EeV neutronsAntennas for the detection of radio emission pulses from cosmic-ray induced air showers at the Pierre Auger ObservatoryMeasurement of the Proton-Air Cross Section ats=57 TeVwith the Pierre Auger ObservatoryA search for anisotropy in the arrival directions of ultra high energy cosmic rays recorded at the Pierre Auger ObservatoryLarge-scale distribution of arrival directions of cosmic rays detected above 10^18^ eV at the Pierre Auger observatorySearch for point-like sources of ultra-high energy neutrinos at the pierre auger observatory and improved limit on the diffuse flux of Tau neutrinosSearch for ultrahigh energy neutrinos in highly inclined events at the Pierre Auger ObservatoryThe exposure of the hybrid detector of the Pierre Auger ObservatorySearch for first harmonic modulation in the right ascension distribution of cosmic rays detected at the Pierre Auger ObservatoryAdvanced functionality for radio analysis in the Offline software framework of the Pierre Auger ObservatoryMeasurement of the Depth of Maximum of Extensive Air Showers above1018 eVTrigger and aperture of the surface detector array of the Pierre Auger ObservatoryAtmospheric effects on extensive air showers observed with the surface detector of the Pierre Auger observatoryLimit on the diffuse flux of ultrahigh energy tau neutrinos with the surface detector of the Pierre Auger ObservatoryUpper limit on the cosmic-ray photon flux above 1019eV using the surface detector of the Pierre Auger ObservatoryUpper Limit on the Diffuse Flux of Ultrahigh Energy Tau Neutrinos from the Pierre Auger ObservatoryMuons in air showers at the Pierre Auger Observatory: Measurement of atmospheric production depthOrigin of atmospheric aerosols at the Pierre Auger Observatory using studies of air mass trajectories in South AmericaProbing the radio emission from air showers with polarization measurementsIdentifying clouds over the Pierre Auger Observatory using infrared satellite dataThe analog signal processing system for the Auger fluorescence detector prototype
P50
Q21521427-6622E98C-D0BB-4E0C-940D-B48FFA32DAD6Q21564041-9EEB5F87-46DD-4AED-954B-5E802B48F3A3Q21564042-A8EDF13D-CFAC-4016-927C-9E47F1A0F0C4Q21564043-3BCDA785-9347-4DD5-9F67-76A753BC6E9CQ21564047-962D2D77-52FD-4AA4-8358-BB048127DE25Q27020452-8ED05EFD-9777-42D8-AE50-D1827F41051BQ27350475-F8A85063-2BDE-4CD1-ADBB-48AD7B3AC0D6Q34712024-E2ED154E-BAB6-4A14-87CB-A59ED4C5821EQ55969171-15548107-2E9E-48C7-85C0-36C501B0FAA4Q57533148-0A11354F-AFC8-41F9-8B07-36CDE35AC48CQ57533212-15F8CEA4-A229-4552-B8A6-1FDE65012EDAQ57616720-0843F120-98CC-4141-AAE4-20AD2D2448AEQ57616725-8F04B4F8-8134-4CA9-B211-DECBBBAB6AD7Q57709458-DDCF09F5-1F11-4B72-94FF-368343C861D5Q57709462-335E5C4E-BFEE-409A-9024-0194A15A3470Q57709462-33A636DA-B2D5-4439-9A56-F6EF6655A451Q57722044-7A6BAAF8-ECA9-41B3-964F-0BDBEBC27AD5Q57722048-5BAFDFA4-5130-4395-BAFB-A2699C8AA167Q57740076-380756FE-CC9A-4D84-8394-819877D2C30DQ57740127-00BFA72D-55EA-4891-A39A-A4A7DEE0C48BQ57740150-4E5AF2E1-629E-4C31-8767-B6D75318A624Q57740154-75EE1DE5-2ED2-495B-B529-B04D957BBA74Q57740170-4C3D67F6-2C43-4D03-A7EE-A028A98481C0Q57740219-AF49DA1D-AF59-48CF-A92C-D45BA1BF2F9FQ57740230-5A5696F8-20EF-40F8-A14B-A74B4895EEE7Q57740247-168D27B8-9020-4460-B219-2E72E1C1014DQ57740281-6A238BA4-3A06-4E81-8FDE-A7C5B3490848Q57740320-33382B9D-F8C6-458C-99E6-7ABB126B8387Q57740359-CB8ECA43-063B-4D59-9F5E-3ABEEE259F06Q57740362-339B44BD-4357-4145-A5B4-CEF42DB86234Q57740430-5061F807-249B-4ED7-A3A6-611E90E4A317Q57740437-A954FD3E-A9F4-413D-8B21-545624E97F61Q57740443-DDB218C6-3DA8-48DC-AB0F-5A5E52F377ACQ57740455-44EAF86A-3EA8-47C6-8F57-CA5181FBDE9CQ57740476-A45EE550-3253-4ED3-A370-7382E3429052Q57740479-37D7B793-3ADD-44BE-9049-369421305EEAQ58302030-27BD8E97-3F38-461B-872F-D2B732F1FFC7Q58315392-751AAE9A-C0C6-4707-B9A0-04F95CBC4A3DQ58315398-29B3CBBE-8792-45A4-853D-A107FD65515BQ58315404-0D4095F6-641D-47A1-B01A-F961E0E366D5
P50
description
researcher
@en
wetenschapper
@nl
հետազոտող
@hy
name
E Menichetti
@ast
E Menichetti
@en
E Menichetti
@es
E Menichetti
@nl
E Menichetti
@sl
type
label
E Menichetti
@ast
E Menichetti
@en
E Menichetti
@es
E Menichetti
@nl
E Menichetti
@sl
prefLabel
E Menichetti
@ast
E Menichetti
@en
E Menichetti
@es
E Menichetti
@nl
E Menichetti
@sl
P106
P31
P496
0000-0001-7143-8200