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...

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Detalles Bibliográficos
Autores: Best S., Bazo Alba J.L.
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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network_acronym_str CONC
network_name_str CONCYTEC-Institucional
repository_id_str 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
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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
score 13.4391
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