A search for point sources of EeV photons
Measurements of air showers made using the hybrid technique developed with the fluorescence and surface detectors of the Pierre Auger Observatory allow a sensitive search for point sources of EeV photons anywhere in the exposed sky. A multivariate analysis reduces the background of hadronic cosmic r...
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Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_0004637X_v789_n2_p_Multitudinario |
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todo:paper_0004637X_v789_n2_p_Multitudinario2023-10-03T14:02:35Z A search for point sources of EeV photons Multitudinario:485 astroparticle physics cosmic rays methods: data analysis Measurements of air showers made using the hybrid technique developed with the fluorescence and surface detectors of the Pierre Auger Observatory allow a sensitive search for point sources of EeV photons anywhere in the exposed sky. A multivariate analysis reduces the background of hadronic cosmic rays. The search is sensitive to a declination band from -85° to +20°, in an energy range from 10 17.3 eV to 10 18.5 eV. No photon point source has been detected. An upper limit on the photon flux has been derived for every direction. The mean value of the energy flux limit that results from this, assuming a photon spectral index of -2, is 0.06 eV cm -2 s -1 , and no celestial direction exceeds 0.25 eV cm -2 s -1 . These upper limits constrain scenarios in which EeV cosmic ray protons are emitted by non-transient sources in the Galaxy. © 2014. The American Astronomical Society. All rights reserved.. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_0004637X_v789_n2_p_Multitudinario |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
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Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
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astroparticle physics cosmic rays methods: data analysis |
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astroparticle physics cosmic rays methods: data analysis Multitudinario:485 A search for point sources of EeV photons |
topic_facet |
astroparticle physics cosmic rays methods: data analysis |
description |
Measurements of air showers made using the hybrid technique developed with the fluorescence and surface detectors of the Pierre Auger Observatory allow a sensitive search for point sources of EeV photons anywhere in the exposed sky. A multivariate analysis reduces the background of hadronic cosmic rays. The search is sensitive to a declination band from -85° to +20°, in an energy range from 10 17.3 eV to 10 18.5 eV. No photon point source has been detected. An upper limit on the photon flux has been derived for every direction. The mean value of the energy flux limit that results from this, assuming a photon spectral index of -2, is 0.06 eV cm -2 s -1 , and no celestial direction exceeds 0.25 eV cm -2 s -1 . These upper limits constrain scenarios in which EeV cosmic ray protons are emitted by non-transient sources in the Galaxy. © 2014. The American Astronomical Society. All rights reserved.. |
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JOUR |
author |
Multitudinario:485 |
author_facet |
Multitudinario:485 |
author_sort |
Multitudinario:485 |
title |
A search for point sources of EeV photons |
title_short |
A search for point sources of EeV photons |
title_full |
A search for point sources of EeV photons |
title_fullStr |
A search for point sources of EeV photons |
title_full_unstemmed |
A search for point sources of EeV photons |
title_sort |
search for point sources of eev photons |
url |
http://hdl.handle.net/20.500.12110/paper_0004637X_v789_n2_p_Multitudinario |
work_keys_str_mv |
AT multitudinario485 asearchforpointsourcesofeevphotons AT multitudinario485 searchforpointsourcesofeevphotons |
_version_ |
1807314399030935552 |