Radio detections towards unidentified variable EGRET sources
- Autores
- Paredes, Josep Maria; Marti, Josep; Ishwara Chandra, C. H.; Torres, Diego F.; Romero, Gustavo Esteban; Combi, Jorge Ariel; Bosch Ramon, Valentí; Muñoz Arjonilla, Álvaro José; Sánchez Sutil, Juan R.
- Año de publicación
- 2008
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Context. A considerable fraction of the gamma-ray sources discovered with the Energetic Gamma-Ray Experiment Telescope (EGRET) remain unidentified. The EGRET sources that have been properly identified are either pulsars or variable sources at both radio and gamma-ray wavelengths. Most of the variable sources are strong radio blazars.However, some low galactic-latitude EGRET sources, with highly variable gamma-ray emission, lack any evident counterpart according to the radio data available until now. Aims. The primary goal of this paper is to identify and characterise the potential radio counterparts of four highly variable gamma-ray sources in the galactic plane through mapping the radio surroundings of the EGRET confidence contours and determining the variable radio sources in the field whenever possible. Methods. We have carried out a radio exploration of the fields of the selected EGRET sources using the Giant Metrewave Radio Telescope (GMRT) interferometer at 21 cm wavelength, with pointings being separated by months. Results. We detected a total of 151 radio sources. Among them, we identified a few radio sources whose flux density has apparently changed on timescales of months. Despite the limitations of our search, their possible variability makes these objects a top-priority target for multiwavelength studies of the potential counterparts of highly variable, unidentified gamma-ray sources.
Fil: Paredes, Josep Maria. Universidad de Barcelona; España
Fil: Marti, Josep. Universidad de Jaén; España
Fil: Ishwara Chandra, C. H.. National Centre for Radio Astrophysics; India
Fil: Torres, Diego F.. Universitat Autònoma de Barcelona; España
Fil: Romero, Gustavo Esteban. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: Combi, Jorge Ariel. Universidad de Jaén; España
Fil: Bosch Ramon, Valentí. Max Planck Institut f¨ur Kernphysik; Alemania
Fil: Muñoz Arjonilla, Álvaro José. Universidad de Jaén; España
Fil: Sánchez Sutil, Juan R.. Universidad de Jaén; España - Materia
-
Radio continuum
Gamma rays
X ray binaries - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/29458
Ver los metadatos del registro completo
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Radio detections towards unidentified variable EGRET sourcesParedes, Josep MariaMarti, JosepIshwara Chandra, C. H.Torres, Diego F.Romero, Gustavo EstebanCombi, Jorge ArielBosch Ramon, ValentíMuñoz Arjonilla, Álvaro JoséSánchez Sutil, Juan R.Radio continuumGamma raysX ray binarieshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Context. A considerable fraction of the gamma-ray sources discovered with the Energetic Gamma-Ray Experiment Telescope (EGRET) remain unidentified. The EGRET sources that have been properly identified are either pulsars or variable sources at both radio and gamma-ray wavelengths. Most of the variable sources are strong radio blazars.However, some low galactic-latitude EGRET sources, with highly variable gamma-ray emission, lack any evident counterpart according to the radio data available until now. Aims. The primary goal of this paper is to identify and characterise the potential radio counterparts of four highly variable gamma-ray sources in the galactic plane through mapping the radio surroundings of the EGRET confidence contours and determining the variable radio sources in the field whenever possible. Methods. We have carried out a radio exploration of the fields of the selected EGRET sources using the Giant Metrewave Radio Telescope (GMRT) interferometer at 21 cm wavelength, with pointings being separated by months. Results. We detected a total of 151 radio sources. Among them, we identified a few radio sources whose flux density has apparently changed on timescales of months. Despite the limitations of our search, their possible variability makes these objects a top-priority target for multiwavelength studies of the potential counterparts of highly variable, unidentified gamma-ray sources.Fil: Paredes, Josep Maria. Universidad de Barcelona; EspañaFil: Marti, Josep. Universidad de Jaén; EspañaFil: Ishwara Chandra, C. H.. National Centre for Radio Astrophysics; IndiaFil: Torres, Diego F.. Universitat Autònoma de Barcelona; EspañaFil: Romero, Gustavo Esteban. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; ArgentinaFil: Combi, Jorge Ariel. Universidad de Jaén; EspañaFil: Bosch Ramon, Valentí. Max Planck Institut f¨ur Kernphysik; AlemaniaFil: Muñoz Arjonilla, Álvaro José. Universidad de Jaén; EspañaFil: Sánchez Sutil, Juan R.. Universidad de Jaén; EspañaEDP Sciences2008-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/29458Paredes, Josep Maria; Marti, Josep; Ishwara Chandra, C. H.; Torres, Diego F.; Romero, Gustavo Esteban; et al.; Radio detections towards unidentified variable EGRET sources; EDP Sciences; Astronomy and Astrophysics; 482; 12-2008; 247-2530004-6361CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20078299info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2008/16/aa8299-07/aa8299-07.htmlinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:30:09Zoai:ri.conicet.gov.ar:11336/29458instacron: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 10:30:09.616CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Radio detections towards unidentified variable EGRET sources |
title |
Radio detections towards unidentified variable EGRET sources |
spellingShingle |
Radio detections towards unidentified variable EGRET sources Paredes, Josep Maria Radio continuum Gamma rays X ray binaries |
title_short |
Radio detections towards unidentified variable EGRET sources |
title_full |
Radio detections towards unidentified variable EGRET sources |
title_fullStr |
Radio detections towards unidentified variable EGRET sources |
title_full_unstemmed |
Radio detections towards unidentified variable EGRET sources |
title_sort |
Radio detections towards unidentified variable EGRET sources |
dc.creator.none.fl_str_mv |
Paredes, Josep Maria Marti, Josep Ishwara Chandra, C. H. Torres, Diego F. Romero, Gustavo Esteban Combi, Jorge Ariel Bosch Ramon, Valentí Muñoz Arjonilla, Álvaro José Sánchez Sutil, Juan R. |
author |
Paredes, Josep Maria |
author_facet |
Paredes, Josep Maria Marti, Josep Ishwara Chandra, C. H. Torres, Diego F. Romero, Gustavo Esteban Combi, Jorge Ariel Bosch Ramon, Valentí Muñoz Arjonilla, Álvaro José Sánchez Sutil, Juan R. |
author_role |
author |
author2 |
Marti, Josep Ishwara Chandra, C. H. Torres, Diego F. Romero, Gustavo Esteban Combi, Jorge Ariel Bosch Ramon, Valentí Muñoz Arjonilla, Álvaro José Sánchez Sutil, Juan R. |
author2_role |
author author author author author author author author |
dc.subject.none.fl_str_mv |
Radio continuum Gamma rays X ray binaries |
topic |
Radio continuum Gamma rays X ray binaries |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
Context. A considerable fraction of the gamma-ray sources discovered with the Energetic Gamma-Ray Experiment Telescope (EGRET) remain unidentified. The EGRET sources that have been properly identified are either pulsars or variable sources at both radio and gamma-ray wavelengths. Most of the variable sources are strong radio blazars.However, some low galactic-latitude EGRET sources, with highly variable gamma-ray emission, lack any evident counterpart according to the radio data available until now. Aims. The primary goal of this paper is to identify and characterise the potential radio counterparts of four highly variable gamma-ray sources in the galactic plane through mapping the radio surroundings of the EGRET confidence contours and determining the variable radio sources in the field whenever possible. Methods. We have carried out a radio exploration of the fields of the selected EGRET sources using the Giant Metrewave Radio Telescope (GMRT) interferometer at 21 cm wavelength, with pointings being separated by months. Results. We detected a total of 151 radio sources. Among them, we identified a few radio sources whose flux density has apparently changed on timescales of months. Despite the limitations of our search, their possible variability makes these objects a top-priority target for multiwavelength studies of the potential counterparts of highly variable, unidentified gamma-ray sources. Fil: Paredes, Josep Maria. Universidad de Barcelona; España Fil: Marti, Josep. Universidad de Jaén; España Fil: Ishwara Chandra, C. H.. National Centre for Radio Astrophysics; India Fil: Torres, Diego F.. Universitat Autònoma de Barcelona; España Fil: Romero, Gustavo Esteban. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina Fil: Combi, Jorge Ariel. Universidad de Jaén; España Fil: Bosch Ramon, Valentí. Max Planck Institut f¨ur Kernphysik; Alemania Fil: Muñoz Arjonilla, Álvaro José. Universidad de Jaén; España Fil: Sánchez Sutil, Juan R.. Universidad de Jaén; España |
description |
Context. A considerable fraction of the gamma-ray sources discovered with the Energetic Gamma-Ray Experiment Telescope (EGRET) remain unidentified. The EGRET sources that have been properly identified are either pulsars or variable sources at both radio and gamma-ray wavelengths. Most of the variable sources are strong radio blazars.However, some low galactic-latitude EGRET sources, with highly variable gamma-ray emission, lack any evident counterpart according to the radio data available until now. Aims. The primary goal of this paper is to identify and characterise the potential radio counterparts of four highly variable gamma-ray sources in the galactic plane through mapping the radio surroundings of the EGRET confidence contours and determining the variable radio sources in the field whenever possible. Methods. We have carried out a radio exploration of the fields of the selected EGRET sources using the Giant Metrewave Radio Telescope (GMRT) interferometer at 21 cm wavelength, with pointings being separated by months. Results. We detected a total of 151 radio sources. Among them, we identified a few radio sources whose flux density has apparently changed on timescales of months. Despite the limitations of our search, their possible variability makes these objects a top-priority target for multiwavelength studies of the potential counterparts of highly variable, unidentified gamma-ray sources. |
publishDate |
2008 |
dc.date.none.fl_str_mv |
2008-12 |
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/11336/29458 Paredes, Josep Maria; Marti, Josep; Ishwara Chandra, C. H.; Torres, Diego F.; Romero, Gustavo Esteban; et al.; Radio detections towards unidentified variable EGRET sources; EDP Sciences; Astronomy and Astrophysics; 482; 12-2008; 247-253 0004-6361 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/29458 |
identifier_str_mv |
Paredes, Josep Maria; Marti, Josep; Ishwara Chandra, C. H.; Torres, Diego F.; Romero, Gustavo Esteban; et al.; Radio detections towards unidentified variable EGRET sources; EDP Sciences; Astronomy and Astrophysics; 482; 12-2008; 247-253 0004-6361 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20078299 info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2008/16/aa8299-07/aa8299-07.html |
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 application/pdf |
dc.publisher.none.fl_str_mv |
EDP Sciences |
publisher.none.fl_str_mv |
EDP Sciences |
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reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
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CONICET Digital (CONICET) |
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CONICET Digital (CONICET) |
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CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
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dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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