An upper limit on the cosmic-ray luminosity of individual sources from gamma-ray observations

Autores
Supanitsky, Alberto Daniel; de Souza, V.
Año de publicación
2013
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Different types of extragalactic objects are known to produce TeV gamma-rays. Some of these objects are the most probable candidates to accelerate cosmic rays up to 1020 eV. It is very well known that gamma-rays can be produced as a result of the cosmic ray propagation through the intergalactic medium. These gamma-rays contribute to the total flux observed in the direction of the source. In this paper we propose a new method to derive an upper limit on the cosmic-ray luminosity of an individual source based on the measured upper limit on the integral flux of GeV-TeV gamma-rays. We show how it is possible to calculate an upper limit on the cosmic-ray luminosity of a particular source and we explore the parameter space in which the current GeV-TeV gamma-ray measurements can offer a useful determination. We study in detail two particular sources, Pictor A and NGC 7469, and we calculate the upper limit on the proton luminosity of each source based on the upper limit on the integral gamma-ray flux measured by the H.E.S.S. telescopes.
Fil: Supanitsky, Alberto Daniel. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: de Souza, V.. Universidade de Sao Paulo; Brasil
Materia
ultra high energy cosmic rays
gamma ray experiments
gamma ray theory
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/17074
Acceder
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network_name_str CONICET Digital (CONICET)
spelling An upper limit on the cosmic-ray luminosity of individual sources from gamma-ray observationsSupanitsky, Alberto Danielde Souza, V.ultra high energy cosmic raysgamma ray experimentsgamma ray theoryhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Different types of extragalactic objects are known to produce TeV gamma-rays. Some of these objects are the most probable candidates to accelerate cosmic rays up to 1020 eV. It is very well known that gamma-rays can be produced as a result of the cosmic ray propagation through the intergalactic medium. These gamma-rays contribute to the total flux observed in the direction of the source. In this paper we propose a new method to derive an upper limit on the cosmic-ray luminosity of an individual source based on the measured upper limit on the integral flux of GeV-TeV gamma-rays. We show how it is possible to calculate an upper limit on the cosmic-ray luminosity of a particular source and we explore the parameter space in which the current GeV-TeV gamma-ray measurements can offer a useful determination. We study in detail two particular sources, Pictor A and NGC 7469, and we calculate the upper limit on the proton luminosity of each source based on the upper limit on the integral gamma-ray flux measured by the H.E.S.S. telescopes.Fil: Supanitsky, Alberto Daniel. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaFil: de Souza, V.. Universidade de Sao Paulo; BrasilIop Publishing2013-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/17074Supanitsky, Alberto Daniel; de Souza, V.; An upper limit on the cosmic-ray luminosity of individual sources from gamma-ray observations; Iop Publishing; Journal Of Cosmology And Astroparticle Physics; 2013; 12-2013; 231-171475-7516enginfo:eu-repo/semantics/altIdentifier/doi/10.1088/1475-7516/2013/12/023info:eu-repo/semantics/altIdentifier/url/iopscience.iop.org/article/10.1088/1475-7516/2013/12/023info:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/1311.4820info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:40:00Zoai:ri.conicet.gov.ar:11336/17074instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 09:40:00.516CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv An upper limit on the cosmic-ray luminosity of individual sources from gamma-ray observations
title An upper limit on the cosmic-ray luminosity of individual sources from gamma-ray observations
spellingShingle An upper limit on the cosmic-ray luminosity of individual sources from gamma-ray observations
Supanitsky, Alberto Daniel
ultra high energy cosmic rays
gamma ray experiments
gamma ray theory
title_short An upper limit on the cosmic-ray luminosity of individual sources from gamma-ray observations
title_full An upper limit on the cosmic-ray luminosity of individual sources from gamma-ray observations
title_fullStr An upper limit on the cosmic-ray luminosity of individual sources from gamma-ray observations
title_full_unstemmed An upper limit on the cosmic-ray luminosity of individual sources from gamma-ray observations
title_sort An upper limit on the cosmic-ray luminosity of individual sources from gamma-ray observations
dc.creator.none.fl_str_mv Supanitsky, Alberto Daniel
de Souza, V.
author Supanitsky, Alberto Daniel
author_facet Supanitsky, Alberto Daniel
de Souza, V.
author_role author
author2 de Souza, V.
author2_role author
dc.subject.none.fl_str_mv ultra high energy cosmic rays
gamma ray experiments
gamma ray theory
topic ultra high energy cosmic rays
gamma ray experiments
gamma ray theory
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Different types of extragalactic objects are known to produce TeV gamma-rays. Some of these objects are the most probable candidates to accelerate cosmic rays up to 1020 eV. It is very well known that gamma-rays can be produced as a result of the cosmic ray propagation through the intergalactic medium. These gamma-rays contribute to the total flux observed in the direction of the source. In this paper we propose a new method to derive an upper limit on the cosmic-ray luminosity of an individual source based on the measured upper limit on the integral flux of GeV-TeV gamma-rays. We show how it is possible to calculate an upper limit on the cosmic-ray luminosity of a particular source and we explore the parameter space in which the current GeV-TeV gamma-ray measurements can offer a useful determination. We study in detail two particular sources, Pictor A and NGC 7469, and we calculate the upper limit on the proton luminosity of each source based on the upper limit on the integral gamma-ray flux measured by the H.E.S.S. telescopes.
Fil: Supanitsky, Alberto Daniel. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: de Souza, V.. Universidade de Sao Paulo; Brasil
description Different types of extragalactic objects are known to produce TeV gamma-rays. Some of these objects are the most probable candidates to accelerate cosmic rays up to 1020 eV. It is very well known that gamma-rays can be produced as a result of the cosmic ray propagation through the intergalactic medium. These gamma-rays contribute to the total flux observed in the direction of the source. In this paper we propose a new method to derive an upper limit on the cosmic-ray luminosity of an individual source based on the measured upper limit on the integral flux of GeV-TeV gamma-rays. We show how it is possible to calculate an upper limit on the cosmic-ray luminosity of a particular source and we explore the parameter space in which the current GeV-TeV gamma-ray measurements can offer a useful determination. We study in detail two particular sources, Pictor A and NGC 7469, and we calculate the upper limit on the proton luminosity of each source based on the upper limit on the integral gamma-ray flux measured by the H.E.S.S. telescopes.
publishDate 2013
dc.date.none.fl_str_mv 2013-12
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/17074
Supanitsky, Alberto Daniel; de Souza, V.; An upper limit on the cosmic-ray luminosity of individual sources from gamma-ray observations; Iop Publishing; Journal Of Cosmology And Astroparticle Physics; 2013; 12-2013; 231-17
1475-7516
url http://hdl.handle.net/11336/17074
identifier_str_mv Supanitsky, Alberto Daniel; de Souza, V.; An upper limit on the cosmic-ray luminosity of individual sources from gamma-ray observations; Iop Publishing; Journal Of Cosmology And Astroparticle Physics; 2013; 12-2013; 231-17
1475-7516
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1088/1475-7516/2013/12/023
info:eu-repo/semantics/altIdentifier/url/iopscience.iop.org/article/10.1088/1475-7516/2013/12/023
info:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/1311.4820
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
application/pdf
dc.publisher.none.fl_str_mv Iop Publishing
publisher.none.fl_str_mv Iop Publishing
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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score 13.070432

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