Výsledky vyhledávání - "Sciutto, Sergio Juan"

The FRAM robotic telescope for atmospheric monitoring at the Pierre Auger Observatory

Autor: Dova, María Teresa, Hansen, Patricia María, Mariazzi, Analisa Gabriela, Sciutto, Sergio Juan, Tueros, Matías Jorge, Vergara Quispe, Indira Dajhana, Wahlberg, Hernán Pablo, The Pierre Auger Collaboration

FRAM (F/Photometric Robotic Atmospheric Monitor) is a robotic telescope operated at the Pierre Auger Observatory in Argentina for the purposes of atmospheric monitoring using stellar photometry. As a passive system which does not produce any light th

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=od______1329::33695406939e3e47ba15fb6be6c993b2
http://sedici.unlp.edu.ar/handle/10915/145162

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Direct measurement of the muonic content of extensive air showers between 2 × 10¹⁷ and 2 × 10¹⁸ eV at the Pierre Auger Observatory

Autor: Calcagni, Laura Randa, Dova, María Teresa, Hansen, Patricia María, Mariazzi, Analisa Gabriela, Sciutto, Sergio Juan, Tueros, Matías Jorge, Vergara Quispe, Indira Dajhana, Wahlberg, Hernán Pablo, The Pierre Auger Collaboration

Publikováno v: SEDICI (UNLP)
Universidad Nacional de La Plata
instacron:UNLP

The hybrid design of the Pierre Auger Observatory allows for the measurement of the properties of extensive air showers initiated by ultra-high energy cosmic rays with unprecedented precision. By using an array of prototype underground muon detectors

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::32a3162f74737b68dbd68a62cd247c3e
http://sedici.unlp.edu.ar/handle/10915/125559

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Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory

The determination of the primary energy of extensive air showers using the uorescence detection technique requires an estimation of the energy carried away by particles that do not deposit all their energy in the atmosphere. This estimation is typica

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=od______1329::74b24f7ebe9cd20d9fbf6cdd3f46e395
http://sedici.unlp.edu.ar/handle/10915/81034

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Limits on point-like sources of ultra-high-energy neutrinos with the Pierre Auger Observatory

With the Surface Detector array (SD) of the Pierre Auger Observatory we can detect neutrinos with energy between 10(¹⁷) eV and 10(²⁰) eV from point-like sources across the sky, from close to the Southern Celestial Pole up to 60° in declination

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=od______1329::4a1613e16fd5769900b32984b778643f
http://sedici.unlp.edu.ar/handle/10915/124305

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Observation of inclined EeV air showers with the radio detector of the Pierre Auger Observatory

With the Auger Engineering Radio Array (AERA) of the Pierre Auger Observatory, we have observed the radio emission from 561 extensive air showers with zenith angles between 60 and 84 . In contrast to air showers with more vertical incidence, these in

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=od______1329::b0affa5df38dfb27de0b09cd46df181d
http://sedici.unlp.edu.ar/handle/10915/113530

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Multi-messenger observations of a binary neutron star merger

Publikováno v: SEDICI (UNLP)
Universidad Nacional de La Plata
instacron:UNLP

On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor inde

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::45000ce7066fdf561760a0259867a585
http://sedici.unlp.edu.ar/handle/10915/87414

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