Search for gamma-ray counterparts of newly discovered radio astrophysical sources
Descripción del Articulo
In this paper we study two newly discovered classes of radio sources: the highly energetic, short-lived events, known as Fast Radio Bursts (FRBs), and a new category of compact sources known as Fanaroff-Riley type 0 radio galaxies (FR0s). Due to a possible catastrophic event origin for the FRBs and...
Autores: | , |
---|---|
Formato: | artículo |
Fecha de Publicación: | 2019 |
Institución: | Consejo Nacional de Ciencia Tecnología e Innovación |
Repositorio: | CONCYTEC-Institucional |
Lenguaje: | inglés |
OAI Identifier: | oai:repositorio.concytec.gob.pe:20.500.12390/2750 |
Enlace del recurso: | https://hdl.handle.net/20.500.12390/2750 https://doi.org/10.22323/1.358.0553 |
Nivel de acceso: | acceso abierto |
Materia: | Radio astronomy Cosmic rays Cosmology Galaxies https://purl.org/pe-repo/ocde/ford#1.03.08 |
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4689 |
dc.title.none.fl_str_mv |
Search for gamma-ray counterparts of newly discovered radio astrophysical sources |
title |
Search for gamma-ray counterparts of newly discovered radio astrophysical sources |
spellingShingle |
Search for gamma-ray counterparts of newly discovered radio astrophysical sources Best S. Radio astronomy Cosmic rays Cosmology Galaxies https://purl.org/pe-repo/ocde/ford#1.03.08 |
title_short |
Search for gamma-ray counterparts of newly discovered radio astrophysical sources |
title_full |
Search for gamma-ray counterparts of newly discovered radio astrophysical sources |
title_fullStr |
Search for gamma-ray counterparts of newly discovered radio astrophysical sources |
title_full_unstemmed |
Search for gamma-ray counterparts of newly discovered radio astrophysical sources |
title_sort |
Search for gamma-ray counterparts of newly discovered radio astrophysical sources |
author |
Best S. |
author_facet |
Best S. Bazo Alba J.L. |
author_role |
author |
author2 |
Bazo Alba J.L. |
author2_role |
author |
dc.contributor.author.fl_str_mv |
Best S. Bazo Alba J.L. |
dc.subject.none.fl_str_mv |
Radio astronomy |
topic |
Radio astronomy Cosmic rays Cosmology Galaxies https://purl.org/pe-repo/ocde/ford#1.03.08 |
dc.subject.es_PE.fl_str_mv |
Cosmic rays Cosmology Galaxies |
dc.subject.ocde.none.fl_str_mv |
https://purl.org/pe-repo/ocde/ford#1.03.08 |
description |
In this paper we study two newly discovered classes of radio sources: the highly energetic, short-lived events, known as Fast Radio Bursts (FRBs), and a new category of compact sources known as Fanaroff-Riley type 0 radio galaxies (FR0s). Due to a possible catastrophic event origin for the FRBs and a previous correlation found with an FR0 in the gamma ray spectrum, it is possible that these radio sources could also emit high energy photons in the Fermi-LAT satellite energy range (20 MeV - 300GeV). Here we present an exhaustive time-dependent and spatial search of all up-to-date observed FRBs and FR0s, respectively. We perform a likelihood analysis of the radio sources by modeling the excess flux of gamma rays with a varying index power law function using data from Fermi-LAT and the 4FGL catalog. Sources with test statistic greater than 16 (corresponding to about 4{\sigma}) were further analyzed including 2 FRBs and 7 FR0s. No correlations with more than 5{\sigma} were found after taking into account nearby sources. Therefore, upper limits for all sources were calculated |
publishDate |
2019 |
dc.date.accessioned.none.fl_str_mv |
2024-05-30T23:13:38Z |
dc.date.available.none.fl_str_mv |
2024-05-30T23:13:38Z |
dc.date.issued.fl_str_mv |
2019 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article |
format |
article |
dc.identifier.uri.none.fl_str_mv |
https://hdl.handle.net/20.500.12390/2750 |
dc.identifier.doi.none.fl_str_mv |
https://doi.org/10.22323/1.358.0553 |
dc.identifier.scopus.none.fl_str_mv |
2-s2.0-85127466653 |
url |
https://hdl.handle.net/20.500.12390/2750 https://doi.org/10.22323/1.358.0553 |
identifier_str_mv |
2-s2.0-85127466653 |
dc.language.iso.none.fl_str_mv |
eng |
language |
eng |
dc.relation.ispartof.none.fl_str_mv |
Proceedings of Science |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess |
dc.rights.uri.none.fl_str_mv |
https://creativecommons.org/licenses/by-nc-nd/4.0/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-nd/4.0/ |
dc.publisher.none.fl_str_mv |
Sissa Medialab Srl |
publisher.none.fl_str_mv |
Sissa Medialab Srl |
dc.source.none.fl_str_mv |
reponame:CONCYTEC-Institucional instname:Consejo Nacional de Ciencia Tecnología e Innovación instacron:CONCYTEC |
instname_str |
Consejo Nacional de Ciencia Tecnología e Innovación |
instacron_str |
CONCYTEC |
institution |
CONCYTEC |
reponame_str |
CONCYTEC-Institucional |
collection |
CONCYTEC-Institucional |
repository.name.fl_str_mv |
Repositorio Institucional CONCYTEC |
repository.mail.fl_str_mv |
repositorio@concytec.gob.pe |
_version_ |
1839175507296387072 |
spelling |
Publicationrp01219600rp07364600Best S.Bazo Alba J.L.2024-05-30T23:13:38Z2024-05-30T23:13:38Z2019https://hdl.handle.net/20.500.12390/2750https://doi.org/10.22323/1.358.05532-s2.0-85127466653In this paper we study two newly discovered classes of radio sources: the highly energetic, short-lived events, known as Fast Radio Bursts (FRBs), and a new category of compact sources known as Fanaroff-Riley type 0 radio galaxies (FR0s). Due to a possible catastrophic event origin for the FRBs and a previous correlation found with an FR0 in the gamma ray spectrum, it is possible that these radio sources could also emit high energy photons in the Fermi-LAT satellite energy range (20 MeV - 300GeV). Here we present an exhaustive time-dependent and spatial search of all up-to-date observed FRBs and FR0s, respectively. We perform a likelihood analysis of the radio sources by modeling the excess flux of gamma rays with a varying index power law function using data from Fermi-LAT and the 4FGL catalog. Sources with test statistic greater than 16 (corresponding to about 4{\sigma}) were further analyzed including 2 FRBs and 7 FR0s. No correlations with more than 5{\sigma} were found after taking into account nearby sources. Therefore, upper limits for all sources were calculatedFondo Nacional de Desarrollo Científico y Tecnológico - FondecytengSissa Medialab SrlProceedings of Scienceinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-nd/4.0/Radio astronomyCosmic rays-1Cosmology-1Galaxies-1https://purl.org/pe-repo/ocde/ford#1.03.08-1Search for gamma-ray counterparts of newly discovered radio astrophysical sourcesinfo:eu-repo/semantics/articlereponame:CONCYTEC-Institucionalinstname:Consejo Nacional de Ciencia Tecnología e Innovacióninstacron:CONCYTEC#PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE#20.500.12390/2750oai:repositorio.concytec.gob.pe:20.500.12390/27502024-05-30 15:42:35.556https://creativecommons.org/licenses/by-nc-nd/4.0/info:eu-repo/semantics/openAccesshttp://purl.org/coar/access_right/c_14cbinfo:eu-repo/semantics/closedAccessmetadata only accesshttps://repositorio.concytec.gob.peRepositorio Institucional CONCYTECrepositorio@concytec.gob.pe#PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE#<Publication xmlns="https://www.openaire.eu/cerif-profile/1.1/" id="3d43121d-b375-4b46-90ed-dee36dda7de8"> <Type xmlns="https://www.openaire.eu/cerif-profile/vocab/COAR_Publication_Types">http://purl.org/coar/resource_type/c_1843</Type> <Language>eng</Language> <Title>Search for gamma-ray counterparts of newly discovered radio astrophysical sources</Title> <PublishedIn> <Publication> <Title>Proceedings of Science</Title> </Publication> </PublishedIn> <PublicationDate>2019</PublicationDate> <DOI>https://doi.org/10.22323/1.358.0553</DOI> <SCP-Number>2-s2.0-85127466653</SCP-Number> <Authors> <Author> <DisplayName>Best S.</DisplayName> <Person id="rp01219" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> <Author> <DisplayName>Bazo Alba J.L.</DisplayName> <Person id="rp07364" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> </Authors> <Editors> </Editors> <Publishers> <Publisher> <DisplayName>Sissa Medialab Srl</DisplayName> <OrgUnit /> </Publisher> </Publishers> <License>https://creativecommons.org/licenses/by-nc-nd/4.0/</License> <Keyword>Radio astronomy</Keyword> <Keyword>Cosmic rays</Keyword> <Keyword>Cosmology</Keyword> <Keyword>Galaxies</Keyword> <Abstract>In this paper we study two newly discovered classes of radio sources: the highly energetic, short-lived events, known as Fast Radio Bursts (FRBs), and a new category of compact sources known as Fanaroff-Riley type 0 radio galaxies (FR0s). Due to a possible catastrophic event origin for the FRBs and a previous correlation found with an FR0 in the gamma ray spectrum, it is possible that these radio sources could also emit high energy photons in the Fermi-LAT satellite energy range (20 MeV - 300GeV). Here we present an exhaustive time-dependent and spatial search of all up-to-date observed FRBs and FR0s, respectively. We perform a likelihood analysis of the radio sources by modeling the excess flux of gamma rays with a varying index power law function using data from Fermi-LAT and the 4FGL catalog. Sources with test statistic greater than 16 (corresponding to about 4{\sigma}) were further analyzed including 2 FRBs and 7 FR0s. No correlations with more than 5{\sigma} were found after taking into account nearby sources. Therefore, upper limits for all sources were calculated</Abstract> <Access xmlns="http://purl.org/coar/access_right" > </Access> </Publication> -1 |
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La información contenida en este registro es de entera responsabilidad de la institución que gestiona el repositorio institucional donde esta contenido este documento o set de datos. El CONCYTEC no se hace responsable por los contenidos (publicaciones y/o datos) accesibles a través del Repositorio Nacional Digital de Ciencia, Tecnología e Innovación de Acceso Abierto (ALICIA).
La información contenida en este registro es de entera responsabilidad de la institución que gestiona el repositorio institucional donde esta contenido este documento o set de datos. El CONCYTEC no se hace responsable por los contenidos (publicaciones y/o datos) accesibles a través del Repositorio Nacional Digital de Ciencia, Tecnología e Innovación de Acceso Abierto (ALICIA).