about
Long term monitoring of the optical background in the Capo Passero deep-sea site with the NEMO tower prototypeOptical and X-ray early follow-up of ANTARES neutrino alertsTime calibration with atmospheric muon tracks in the ANTARES neutrino telescopeSperm whale long-range echolocation sounds revealed by ANTARES, a deep-sea neutrino telescope.Deep-sea bioluminescence blooms after dense water formation at the ocean surface.An algorithm for the reconstruction of high-energy neutrino-induced particle showers and its application to the ANTARES neutrino telescope.Abyssal undular vortices in the Eastern Mediterranean basin.High-energy neutrino follow-up search of gravitational wave event GW150914 with ANTARES and IceCubeA polarized fast radio burst at low Galactic latitudeSearch for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger ObservatoryA first search for coincident gravitational waves and high energy neutrinos using LIGO, Virgo and ANTARES data from 2007Search for high-energy neutrinos from gravitational wave event GW151226 and candidate LVT151012 with ANTARES and IceCubeAll-flavor Search for a Diffuse Flux of Cosmic Neutrinos with Nine Years of ANTARES DataAn Algorithm for the Reconstruction of Neutrino-induced Showers in the ANTARES Neutrino TelescopeThe SUrvey for Pulsars and Extragalactic Radio Bursts – II. New FRB discoveries and their follow-upAll-sky search for high-energy neutrinos from gravitational wave event GW170104 with the Antares neutrino telescopeFirst all-flavor neutrino pointlike source search with the ANTARES neutrino telescopeNew constraints on all flavor Galactic diffuse neutrino emission with the ANTARES telescopeSearch for relativistic magnetic monopoles with five years of the ANTARES detector dataThe first combined search for neutrino point-sources in the southern hemisphere with the ANTARES and IceCube neutrino telescopesNEMO-SN1 Abyssal Cabled Observatory in the Western Ionian SeaNEMO-SN1 (Western Ionian Sea, off Eastern Sicily): Example of architecture of a cabled observatoryDeep sea tests of a prototype of the KM3NeT digital optical moduleDetection potential of the KM3NeT detector for high-energy neutrinos from the Fermi bubblesANTARES: The first undersea neutrino telescopeStudies of a full-scale mechanical prototype line for the ANTARES neutrino telescope and tests of a prototype instrument for deep-sea acoustic measurementsThe ANTARES optical beacon systemThe data acquisition system for the ANTARES neutrino telescopeFirst results of the Instrumentation Line for the deep-sea ANTARES neutrino telescopeStudy of large hemispherical photomultiplier tubes for the ANTARES neutrino telescopeIntrinsic limits on resolutions in muon- and electron-neutrino charged-current events in the KM3NeT/ORCA detectorLetter of intent for KM3NeT 2.0The ANTARES optical moduleSedimentation and fouling of optical surfaces at the ANTARES siteSearch for high-energy neutrinos from bright GRBs with ANTARESSearch for dark matter annihilation in the earth using the ANTARES neutrino telescopeResults from the search for dark matter in the Milky Way with 9 years of data of the ANTARES neutrino telescopeStacked search for time shifted high energy neutrinos from gamma ray bursts with the Antares neutrino telescopeTime-dependent search for neutrino emission from X-ray binaries with the ANTARES telescopeMurchison widefield array limits on radio emission from ANTARES neutrino events
P50
Q27013033-CAA095D0-178E-4DF5-8A23-8D38DFBFF605Q27016655-6858E87E-EEAE-4447-B247-9BB42FB72EECQ27019807-68DE1829-4EE1-466F-9B88-A29D4B691578Q30358744-16B40CED-997D-4719-9BBE-C01F19D2CA19Q30452103-A73E15DE-2DC5-41AE-A435-ED520B259806Q38642117-2211C63A-0085-49F7-9DAD-EEC4CC9E6483Q39118368-A6A17FB3-3D9A-418C-BAA4-229ECBD86CD5Q40907274-B132BD19-60F0-45BA-AF50-BA4016CF3B80Q56001051-F24E4FC3-A939-4C90-9028-8F7B44ED7B44Q56595381-E25A0107-C30A-4FFF-AF1D-A0762C43B61AQ56977659-11B1E4DB-9CCB-4C06-86B9-548E94B89A90Q57561994-790A220C-A8ED-4D12-BAC6-CD187B23B684Q57723217-1A9F9976-2462-4ACB-BB4A-5772212BD25CQ57723222-43A448D2-345A-4412-9CF2-328FDC722BC2Q57723226-F858739D-7182-47DA-9494-ADB2BB28ABCBQ57723230-9A7719F4-0908-4F0D-9853-F37E97106E57Q57723233-76CD3B63-7DDC-4BDC-A330-B4F45806BDAEQ57723237-EB957678-02EB-457A-8EB5-8388778B1DD3Q57723244-EF8DA305-2418-4C19-B203-DE3AEDEC40E9Q57739831-F7F80161-4B5B-40A5-8D14-FB78FF3AAA31Q57858684-CA1FA393-7C12-4CA3-8142-98EF5D1CDA0CQ57858702-DE547D10-D3EF-4ED8-A2DA-BA79EC1456B0Q58046208-DA8FDA44-C543-4B52-AB37-576D76F940CEQ58046268-CD4E65F9-F7CB-423D-9502-9A67A6AB6F59Q58203187-68B9F41D-9446-4044-864D-6FC17B483B81Q58203231-EB59B5F6-F8E9-42FA-A5C0-72D6EFDF73CDQ58203233-15C09E15-ED99-4D3A-9CA6-A031CE91BEAFQ58203235-A720B003-56DF-4D20-A85A-C2B15752A0A5Q58203243-2717F602-BA08-478B-B973-60AB54B1BDC0Q58203253-D2F8E000-1DD6-4F3D-83BF-29F87CB8FAA6Q58323476-D42BEBED-69B4-4819-9286-A2554A7CF5A9Q58323477-472B49ED-45F1-4DFF-9CF4-CE9D1DD0900BQ58323507-B0DB5C8E-3FCA-42F0-B2C0-E8EB2354A6E5Q58341369-EF978E7F-C3D7-4C63-8CCE-473A5932DB17Q58341441-9C7E55AA-5F10-450A-B43E-7A9186142ABFQ58341446-32E34BF4-C4F5-454E-813B-07EE3185E80CQ58341452-E9E81B4A-DB72-4265-A945-B5BA67CD51CAQ58341456-7990768E-F9D2-4A3B-BFD4-BDC669F6B9DDQ58341459-46611472-1506-41D0-B101-6766B3A58E87Q58341473-CC5E9471-784E-4258-BF04-FFA200DFD603
P50
description
researcher
@en
wetenschapper
@nl
հետազոտող
@hy
name
P. Piattelli
@nl
Paolo Piattelli
@en
Paolo Piattelli
@es
type
label
P. Piattelli
@nl
Paolo Piattelli
@en
Paolo Piattelli
@es
altLabel
P. Piattelli
@en
prefLabel
P. Piattelli
@nl
Paolo Piattelli
@en
Paolo Piattelli
@es
P106
P1153
6701516602
P21
P31
P496
0000-0003-4748-6485