Erratum: "Search for dark matter annihilation signals from the Fornax Galaxy Cluster with H.E.S.S."

Autores
Medina, Maria Clementina; Hess Collaboration
Año de publicación
2014
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
In the article by Abramowski et al. (2012), H.E.S.S. observations of the Fornax galaxy cluster were used to produce exclusion limits on a dark matter (DM) annihilation γ -ray signal. Upper limits on the velocity-weighted annihilation cross section (σ v) as a function of the DM particle mass were computed. Constraints were derived for different DM particle models, such as those arising from supersymmetric models, and various annihilation final states were considered. Here we report on three independent problems identified with some of the figures and DM annihilation spectra used in that article
Fil: Medina, Maria Clementina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto Argentino de Radioastronomia (i); Argentina. Institut de Recherche sur les lois Fondamentales de l; Francia
Fil: Hess Collaboration.
Materia
Gamma-Rays
Dark Ennergy
Annihilation
Fornax Galaxy
Dark Matter Annihilation
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:11336/4646
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/4646
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Erratum: "Search for dark matter annihilation signals from the Fornax Galaxy Cluster with H.E.S.S."Medina, Maria ClementinaHess CollaborationGamma-RaysDark EnnergyAnnihilationFornax GalaxyDark Matter Annihilationhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1In the article by Abramowski et al. (2012), H.E.S.S. observations of the Fornax galaxy cluster were used to produce exclusion limits on a dark matter (DM) annihilation γ -ray signal. Upper limits on the velocity-weighted annihilation cross section (σ v) as a function of the DM particle mass were computed. Constraints were derived for different DM particle models, such as those arising from supersymmetric models, and various annihilation final states were considered. Here we report on three independent problems identified with some of the figures and DM annihilation spectra used in that articleFil: Medina, Maria Clementina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto Argentino de Radioastronomia (i); Argentina. Institut de Recherche sur les lois Fondamentales de l; FranciaFil: Hess Collaboration.IOP Publishing2014-03info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/4646Medina, Maria Clementina; Hess Collaboration; Erratum: "Search for dark matter annihilation signals from the Fornax Galaxy Cluster with H.E.S.S."; IOP Publishing; Astrophysical Journal; 750; 1; 3-2014; 63-670004-637Xenghttp://dx.doi.org/10.1088/0004-637X/750/2/123info:eu-repo/semantics/altIdentifier/doi/10.1088/0004-637X/783/1/63info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/0004-637X/783/1/63/metainfo:eu-repo/semantics/altIdentifier/issn/0004-637Xinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:57:18Zoai:ri.conicet.gov.ar:11336/4646instacron: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 09:57:19.158CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Erratum: "Search for dark matter annihilation signals from the Fornax Galaxy Cluster with H.E.S.S."
title Erratum: "Search for dark matter annihilation signals from the Fornax Galaxy Cluster with H.E.S.S."
spellingShingle Erratum: "Search for dark matter annihilation signals from the Fornax Galaxy Cluster with H.E.S.S."
Medina, Maria Clementina
Gamma-Rays
Dark Ennergy
Annihilation
Fornax Galaxy
Dark Matter Annihilation
title_short Erratum: "Search for dark matter annihilation signals from the Fornax Galaxy Cluster with H.E.S.S."
title_full Erratum: "Search for dark matter annihilation signals from the Fornax Galaxy Cluster with H.E.S.S."
title_fullStr Erratum: "Search for dark matter annihilation signals from the Fornax Galaxy Cluster with H.E.S.S."
title_full_unstemmed Erratum: "Search for dark matter annihilation signals from the Fornax Galaxy Cluster with H.E.S.S."
title_sort Erratum: "Search for dark matter annihilation signals from the Fornax Galaxy Cluster with H.E.S.S."
dc.creator.none.fl_str_mv Medina, Maria Clementina
Hess Collaboration
author Medina, Maria Clementina
author_facet Medina, Maria Clementina
Hess Collaboration
author_role author
author2 Hess Collaboration
author2_role author
dc.subject.none.fl_str_mv Gamma-Rays
Dark Ennergy
Annihilation
Fornax Galaxy
Dark Matter Annihilation
topic Gamma-Rays
Dark Ennergy
Annihilation
Fornax Galaxy
Dark Matter Annihilation
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv In the article by Abramowski et al. (2012), H.E.S.S. observations of the Fornax galaxy cluster were used to produce exclusion limits on a dark matter (DM) annihilation γ -ray signal. Upper limits on the velocity-weighted annihilation cross section (σ v) as a function of the DM particle mass were computed. Constraints were derived for different DM particle models, such as those arising from supersymmetric models, and various annihilation final states were considered. Here we report on three independent problems identified with some of the figures and DM annihilation spectra used in that article
Fil: Medina, Maria Clementina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto Argentino de Radioastronomia (i); Argentina. Institut de Recherche sur les lois Fondamentales de l; Francia
Fil: Hess Collaboration.
description In the article by Abramowski et al. (2012), H.E.S.S. observations of the Fornax galaxy cluster were used to produce exclusion limits on a dark matter (DM) annihilation γ -ray signal. Upper limits on the velocity-weighted annihilation cross section (σ v) as a function of the DM particle mass were computed. Constraints were derived for different DM particle models, such as those arising from supersymmetric models, and various annihilation final states were considered. Here we report on three independent problems identified with some of the figures and DM annihilation spectra used in that article
publishDate 2014
dc.date.none.fl_str_mv 2014-03
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/11336/4646
Medina, Maria Clementina; Hess Collaboration; Erratum: "Search for dark matter annihilation signals from the Fornax Galaxy Cluster with H.E.S.S."; IOP Publishing; Astrophysical Journal; 750; 1; 3-2014; 63-67
0004-637X
url http://hdl.handle.net/11336/4646
identifier_str_mv Medina, Maria Clementina; Hess Collaboration; Erratum: "Search for dark matter annihilation signals from the Fornax Galaxy Cluster with H.E.S.S."; IOP Publishing; Astrophysical Journal; 750; 1; 3-2014; 63-67
0004-637X
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv http://dx.doi.org/10.1088/0004-637X/750/2/123
info:eu-repo/semantics/altIdentifier/doi/10.1088/0004-637X/783/1/63
info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/0004-637X/783/1/63/meta
info:eu-repo/semantics/altIdentifier/issn/0004-637X
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
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
_version_ 1844613715149717504
score 13.070432

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