A Search for Ultra-high-energy Neutrinos from TXS 0506+056 Using the Pierre Auger Observatory

Results of a search for ultra-high-energy neutrinos with the Pierre Auger Observatory from the direction of the blazar TXS 0506+056 are presented. They were obtained as part of the follow-up that stemmed from the detection of high-energy neutrinos and gamma rays with IceCube, Fermi-LAT, MAGIC, and o...

Descripción completa

Detalles Bibliográficos
Autores principales: 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
Formato: Articulo
Lenguaje:Inglés
Publicado: 2020
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/146513
Aporte de:
id I19-R120-10915-146513
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Física
spellingShingle Física
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
A Search for Ultra-high-energy Neutrinos from TXS 0506+056 Using the Pierre Auger Observatory
topic_facet Física
description Results of a search for ultra-high-energy neutrinos with the Pierre Auger Observatory from the direction of the blazar TXS 0506+056 are presented. They were obtained as part of the follow-up that stemmed from the detection of high-energy neutrinos and gamma rays with IceCube, Fermi-LAT, MAGIC, and other detectors of electromagnetic radiation in several bands. The Pierre Auger Observatory is sensitive to neutrinos in the energy range from 100 PeV to 100 EeV and in the zenith-angle range from θ = 60° to θ = 95°, where the zenith angle is measured from the vertical direction. No neutrinos from the direction of TXS 0506+056 have been found. The results were analyzed in three periods: One of 6 months around the detection of IceCube-170922 A, coinciding with a flare period of TXS 0506+056, a second one of 110 days during which the IceCube collaboration found an excess of 13 neutrinos from a direction compatible with TXS 0506+056, and a third one from 2004 January 1 up to 2018 August 31, over which the Pierre Auger Observatory has been taking data. The sensitivity of the Observatory is addressed for different spectral indices by considering the fluxes that would induce a single expected event during the observation period. For indices compatible with those measured by the IceCube collaboration the expected number of neutrinos at the Observatory is well below one. Spectral indices as hard as 1.5 would have to apply in this energy range to expect a single event to have been detected.
format Articulo
Articulo
author 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
author_facet 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
author_sort Calcagni, Laura Randa
title A Search for Ultra-high-energy Neutrinos from TXS 0506+056 Using the Pierre Auger Observatory
title_short A Search for Ultra-high-energy Neutrinos from TXS 0506+056 Using the Pierre Auger Observatory
title_full A Search for Ultra-high-energy Neutrinos from TXS 0506+056 Using the Pierre Auger Observatory
title_fullStr A Search for Ultra-high-energy Neutrinos from TXS 0506+056 Using the Pierre Auger Observatory
title_full_unstemmed A Search for Ultra-high-energy Neutrinos from TXS 0506+056 Using the Pierre Auger Observatory
title_sort search for ultra-high-energy neutrinos from txs 0506+056 using the pierre auger observatory
publishDate 2020
url http://sedici.unlp.edu.ar/handle/10915/146513
work_keys_str_mv AT calcagnilauraranda asearchforultrahighenergyneutrinosfromtxs0506056usingthepierreaugerobservatory
AT dovamariateresa asearchforultrahighenergyneutrinosfromtxs0506056usingthepierreaugerobservatory
AT hansenpatriciamaria asearchforultrahighenergyneutrinosfromtxs0506056usingthepierreaugerobservatory
AT mariazzianalisagabriela asearchforultrahighenergyneutrinosfromtxs0506056usingthepierreaugerobservatory
AT sciuttosergiojuan asearchforultrahighenergyneutrinosfromtxs0506056usingthepierreaugerobservatory
AT tuerosmatiasjorge asearchforultrahighenergyneutrinosfromtxs0506056usingthepierreaugerobservatory
AT vergaraquispeindiradajhana asearchforultrahighenergyneutrinosfromtxs0506056usingthepierreaugerobservatory
AT wahlberghernanpablo asearchforultrahighenergyneutrinosfromtxs0506056usingthepierreaugerobservatory
AT thepierreaugercollaboration asearchforultrahighenergyneutrinosfromtxs0506056usingthepierreaugerobservatory
AT calcagnilauraranda searchforultrahighenergyneutrinosfromtxs0506056usingthepierreaugerobservatory
AT dovamariateresa searchforultrahighenergyneutrinosfromtxs0506056usingthepierreaugerobservatory
AT hansenpatriciamaria searchforultrahighenergyneutrinosfromtxs0506056usingthepierreaugerobservatory
AT mariazzianalisagabriela searchforultrahighenergyneutrinosfromtxs0506056usingthepierreaugerobservatory
AT sciuttosergiojuan searchforultrahighenergyneutrinosfromtxs0506056usingthepierreaugerobservatory
AT tuerosmatiasjorge searchforultrahighenergyneutrinosfromtxs0506056usingthepierreaugerobservatory
AT vergaraquispeindiradajhana searchforultrahighenergyneutrinosfromtxs0506056usingthepierreaugerobservatory
AT wahlberghernanpablo searchforultrahighenergyneutrinosfromtxs0506056usingthepierreaugerobservatory
AT thepierreaugercollaboration searchforultrahighenergyneutrinosfromtxs0506056usingthepierreaugerobservatory
bdutipo_str Repositorios
_version_ 1764820461372309504