Powerful Radio Sources in the Southern Sky. II. A Swift X-Ray Perspective
- Autores
- Massaro, F.; White, S. V.; Paggi, A.; Jimenez Gallardo, A.; Madrid, J. P.; Mazzucchelli, C.; Forman, W. R.; Capetti, A.; Leto, C.; García Pérez, A.; Cheung, C. C.; Chavushyan, V.; Nesvadba, N. P. H.; Andruchow, Ileana; Peña Herazo, H.A.; Sani, E.; Grossová, R.; Reynaldi, María Victoria; Kraft, R. P.; Balmaverde, B.; Cellone, Sergio Aldo
- Año de publicación
- 2023
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We recently constructed the G4Jy-3CRE, a catalog of extragalactic radio sources based on the GLEAM 4-Jy (G4Jy) sample, with the aim of increasing the number of powerful radio galaxies and quasars with similar selection criteria to those of the revised release of the Third Cambridge Catalog (3CR). The G4Jy-3CRE consists of a total of 264 radio sources mainly visible from the Southern Hemisphere. Here, we present an initial X-ray analysis of 89 G4Jy-3CRE radio sources with archival X-ray observations from the Neil Gehrels Swift Observatory. We reduced a total of 624 Swift observations, for about 0.9 Ms of integrated exposure time. We found X-ray counterparts for 59 radio sources belonging to the G4Jy-3CRE, nine of them showing extended X-ray emission. The remaining 30 sources do not show any X-ray emission associated with their radio cores. Our analysis demonstrates that X-ray snapshot observations, even if lacking uniform exposure times, as those carried out with Swift, allow us to (i) verify and/or refine the host galaxy identification; (ii) discover the extended X-ray emission around radio galaxies of the intracluster medium when harbored in galaxy clusters, as the case of G4Jy 1518 and G4Jy 1664; and (iii) detect X-ray radiation arising from their radio lobes, as for G4Jy 1863.
Fil: Massaro, F.. Università di Torino; Italia
Fil: White, S. V.. Istituto Nazionale di Astrofisica; Italia
Fil: Paggi, A.. Università di Torino; Italia
Fil: Jimenez Gallardo, A.. Università di Torino; Italia
Fil: Madrid, J. P.. University of Texas; Estados Unidos
Fil: Mazzucchelli, C.. Università di Torino; Italia
Fil: Forman, W. R.. No especifíca;
Fil: Capetti, A.. Istituto Nazionale di Astrofisica; Italia
Fil: Leto, C.. Università di Torino; Italia
Fil: García Pérez, A.. Universidad de Bologna; Italia
Fil: Cheung, C. C.. Istituto Nazionale di Astrofisica; Italia
Fil: Chavushyan, V.. No especifíca;
Fil: Nesvadba, N. P. H.. Universidad Diego Portales; Chile
Fil: Andruchow, Ileana. 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. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Peña Herazo, H.A.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Sani, E.. Istituto Nazionale di Astrofisica; Italia
Fil: Grossová, R.. Masaryk University; República Checa
Fil: Reynaldi, María Victoria. Università di Torino; Italia. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Kraft, R. P.. Instituto Nacional de Astrofisica Optica y Electronica; México
Fil: Balmaverde, B.. Spece Sciences División. Naval Research Laboratory; Estados Unidos
Fil: Cellone, Sergio Aldo. Harvard-Smithsonian Center for Astrophysics; Estados Unidos. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina - Materia
-
RADIO ACTIVE NUCLEI (2134)
RADIO JETS (1347)
RADIO LOBES (1348)
RADIO LOUD QUASARS (1349)
GALAXY CLUSTERS (584)
GALACTIC AND EXTRAGALACTICA ASTRONOMY (563)
X-RAY SURVEYS (1824)
SURVEYS (1671) - 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:11336/256408
Ver los metadatos del registro completo
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oai:ri.conicet.gov.ar:11336/256408 |
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Powerful Radio Sources in the Southern Sky. II. A Swift X-Ray PerspectiveMassaro, F.White, S. V.Paggi, A.Jimenez Gallardo, A.Madrid, J. P.Mazzucchelli, C.Forman, W. R.Capetti, A.Leto, C.García Pérez, A.Cheung, C. C.Chavushyan, V.Nesvadba, N. P. H.Andruchow, IleanaPeña Herazo, H.A.Sani, E.Grossová, R.Reynaldi, María VictoriaKraft, R. P.Balmaverde, B.Cellone, Sergio AldoRADIO ACTIVE NUCLEI (2134)RADIO JETS (1347)RADIO LOBES (1348)RADIO LOUD QUASARS (1349)GALAXY CLUSTERS (584)GALACTIC AND EXTRAGALACTICA ASTRONOMY (563)X-RAY SURVEYS (1824)SURVEYS (1671)https://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We recently constructed the G4Jy-3CRE, a catalog of extragalactic radio sources based on the GLEAM 4-Jy (G4Jy) sample, with the aim of increasing the number of powerful radio galaxies and quasars with similar selection criteria to those of the revised release of the Third Cambridge Catalog (3CR). The G4Jy-3CRE consists of a total of 264 radio sources mainly visible from the Southern Hemisphere. Here, we present an initial X-ray analysis of 89 G4Jy-3CRE radio sources with archival X-ray observations from the Neil Gehrels Swift Observatory. We reduced a total of 624 Swift observations, for about 0.9 Ms of integrated exposure time. We found X-ray counterparts for 59 radio sources belonging to the G4Jy-3CRE, nine of them showing extended X-ray emission. The remaining 30 sources do not show any X-ray emission associated with their radio cores. Our analysis demonstrates that X-ray snapshot observations, even if lacking uniform exposure times, as those carried out with Swift, allow us to (i) verify and/or refine the host galaxy identification; (ii) discover the extended X-ray emission around radio galaxies of the intracluster medium when harbored in galaxy clusters, as the case of G4Jy 1518 and G4Jy 1664; and (iii) detect X-ray radiation arising from their radio lobes, as for G4Jy 1863.Fil: Massaro, F.. Università di Torino; ItaliaFil: White, S. V.. Istituto Nazionale di Astrofisica; ItaliaFil: Paggi, A.. Università di Torino; ItaliaFil: Jimenez Gallardo, A.. Università di Torino; ItaliaFil: Madrid, J. P.. University of Texas; Estados UnidosFil: Mazzucchelli, C.. Università di Torino; ItaliaFil: Forman, W. R.. No especifíca;Fil: Capetti, A.. Istituto Nazionale di Astrofisica; ItaliaFil: Leto, C.. Università di Torino; ItaliaFil: García Pérez, A.. Universidad de Bologna; ItaliaFil: Cheung, C. C.. Istituto Nazionale di Astrofisica; ItaliaFil: Chavushyan, V.. No especifíca;Fil: Nesvadba, N. P. H.. Universidad Diego Portales; ChileFil: Andruchow, Ileana. 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. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: Peña Herazo, H.A.. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Sani, E.. Istituto Nazionale di Astrofisica; ItaliaFil: Grossová, R.. Masaryk University; República ChecaFil: Reynaldi, María Victoria. Università di Torino; Italia. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaFil: Kraft, R. P.. Instituto Nacional de Astrofisica Optica y Electronica; MéxicoFil: Balmaverde, B.. Spece Sciences División. Naval Research Laboratory; Estados UnidosFil: Cellone, Sergio Aldo. Harvard-Smithsonian Center for Astrophysics; Estados Unidos. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaIOP Publishing2023-09info: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/11336/256408Massaro, F.; White, S. V.; Paggi, A.; Jimenez Gallardo, A.; Madrid, J. P.; et al.; Powerful Radio Sources in the Southern Sky. II. A Swift X-Ray Perspective; IOP Publishing; Astrophysical Journal Supplement Series; 268; 1; 9-2023; 32-490067-0049CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4365/ace1f5info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4365/ace1f5info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-15T14:59:34Zoai:ri.conicet.gov.ar:11336/256408instacron: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:34982025-10-15 14:59:34.418CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Powerful Radio Sources in the Southern Sky. II. A Swift X-Ray Perspective |
title |
Powerful Radio Sources in the Southern Sky. II. A Swift X-Ray Perspective |
spellingShingle |
Powerful Radio Sources in the Southern Sky. II. A Swift X-Ray Perspective Massaro, F. RADIO ACTIVE NUCLEI (2134) RADIO JETS (1347) RADIO LOBES (1348) RADIO LOUD QUASARS (1349) GALAXY CLUSTERS (584) GALACTIC AND EXTRAGALACTICA ASTRONOMY (563) X-RAY SURVEYS (1824) SURVEYS (1671) |
title_short |
Powerful Radio Sources in the Southern Sky. II. A Swift X-Ray Perspective |
title_full |
Powerful Radio Sources in the Southern Sky. II. A Swift X-Ray Perspective |
title_fullStr |
Powerful Radio Sources in the Southern Sky. II. A Swift X-Ray Perspective |
title_full_unstemmed |
Powerful Radio Sources in the Southern Sky. II. A Swift X-Ray Perspective |
title_sort |
Powerful Radio Sources in the Southern Sky. II. A Swift X-Ray Perspective |
dc.creator.none.fl_str_mv |
Massaro, F. White, S. V. Paggi, A. Jimenez Gallardo, A. Madrid, J. P. Mazzucchelli, C. Forman, W. R. Capetti, A. Leto, C. García Pérez, A. Cheung, C. C. Chavushyan, V. Nesvadba, N. P. H. Andruchow, Ileana Peña Herazo, H.A. Sani, E. Grossová, R. Reynaldi, María Victoria Kraft, R. P. Balmaverde, B. Cellone, Sergio Aldo |
author |
Massaro, F. |
author_facet |
Massaro, F. White, S. V. Paggi, A. Jimenez Gallardo, A. Madrid, J. P. Mazzucchelli, C. Forman, W. R. Capetti, A. Leto, C. García Pérez, A. Cheung, C. C. Chavushyan, V. Nesvadba, N. P. H. Andruchow, Ileana Peña Herazo, H.A. Sani, E. Grossová, R. Reynaldi, María Victoria Kraft, R. P. Balmaverde, B. Cellone, Sergio Aldo |
author_role |
author |
author2 |
White, S. V. Paggi, A. Jimenez Gallardo, A. Madrid, J. P. Mazzucchelli, C. Forman, W. R. Capetti, A. Leto, C. García Pérez, A. Cheung, C. C. Chavushyan, V. Nesvadba, N. P. H. Andruchow, Ileana Peña Herazo, H.A. Sani, E. Grossová, R. Reynaldi, María Victoria Kraft, R. P. Balmaverde, B. Cellone, Sergio Aldo |
author2_role |
author author author author author author author author author author author author author author author author author author author author |
dc.subject.none.fl_str_mv |
RADIO ACTIVE NUCLEI (2134) RADIO JETS (1347) RADIO LOBES (1348) RADIO LOUD QUASARS (1349) GALAXY CLUSTERS (584) GALACTIC AND EXTRAGALACTICA ASTRONOMY (563) X-RAY SURVEYS (1824) SURVEYS (1671) |
topic |
RADIO ACTIVE NUCLEI (2134) RADIO JETS (1347) RADIO LOBES (1348) RADIO LOUD QUASARS (1349) GALAXY CLUSTERS (584) GALACTIC AND EXTRAGALACTICA ASTRONOMY (563) X-RAY SURVEYS (1824) SURVEYS (1671) |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
We recently constructed the G4Jy-3CRE, a catalog of extragalactic radio sources based on the GLEAM 4-Jy (G4Jy) sample, with the aim of increasing the number of powerful radio galaxies and quasars with similar selection criteria to those of the revised release of the Third Cambridge Catalog (3CR). The G4Jy-3CRE consists of a total of 264 radio sources mainly visible from the Southern Hemisphere. Here, we present an initial X-ray analysis of 89 G4Jy-3CRE radio sources with archival X-ray observations from the Neil Gehrels Swift Observatory. We reduced a total of 624 Swift observations, for about 0.9 Ms of integrated exposure time. We found X-ray counterparts for 59 radio sources belonging to the G4Jy-3CRE, nine of them showing extended X-ray emission. The remaining 30 sources do not show any X-ray emission associated with their radio cores. Our analysis demonstrates that X-ray snapshot observations, even if lacking uniform exposure times, as those carried out with Swift, allow us to (i) verify and/or refine the host galaxy identification; (ii) discover the extended X-ray emission around radio galaxies of the intracluster medium when harbored in galaxy clusters, as the case of G4Jy 1518 and G4Jy 1664; and (iii) detect X-ray radiation arising from their radio lobes, as for G4Jy 1863. Fil: Massaro, F.. Università di Torino; Italia Fil: White, S. V.. Istituto Nazionale di Astrofisica; Italia Fil: Paggi, A.. Università di Torino; Italia Fil: Jimenez Gallardo, A.. Università di Torino; Italia Fil: Madrid, J. P.. University of Texas; Estados Unidos Fil: Mazzucchelli, C.. Università di Torino; Italia Fil: Forman, W. R.. No especifíca; Fil: Capetti, A.. Istituto Nazionale di Astrofisica; Italia Fil: Leto, C.. Università di Torino; Italia Fil: García Pérez, A.. Universidad de Bologna; Italia Fil: Cheung, C. C.. Istituto Nazionale di Astrofisica; Italia Fil: Chavushyan, V.. No especifíca; Fil: Nesvadba, N. P. H.. Universidad Diego Portales; Chile Fil: Andruchow, Ileana. 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. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina Fil: Peña Herazo, H.A.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos Fil: Sani, E.. Istituto Nazionale di Astrofisica; Italia Fil: Grossová, R.. Masaryk University; República Checa Fil: Reynaldi, María Victoria. Università di Torino; Italia. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina Fil: Kraft, R. P.. Instituto Nacional de Astrofisica Optica y Electronica; México Fil: Balmaverde, B.. Spece Sciences División. Naval Research Laboratory; Estados Unidos Fil: Cellone, Sergio Aldo. Harvard-Smithsonian Center for Astrophysics; Estados Unidos. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina |
description |
We recently constructed the G4Jy-3CRE, a catalog of extragalactic radio sources based on the GLEAM 4-Jy (G4Jy) sample, with the aim of increasing the number of powerful radio galaxies and quasars with similar selection criteria to those of the revised release of the Third Cambridge Catalog (3CR). The G4Jy-3CRE consists of a total of 264 radio sources mainly visible from the Southern Hemisphere. Here, we present an initial X-ray analysis of 89 G4Jy-3CRE radio sources with archival X-ray observations from the Neil Gehrels Swift Observatory. We reduced a total of 624 Swift observations, for about 0.9 Ms of integrated exposure time. We found X-ray counterparts for 59 radio sources belonging to the G4Jy-3CRE, nine of them showing extended X-ray emission. The remaining 30 sources do not show any X-ray emission associated with their radio cores. Our analysis demonstrates that X-ray snapshot observations, even if lacking uniform exposure times, as those carried out with Swift, allow us to (i) verify and/or refine the host galaxy identification; (ii) discover the extended X-ray emission around radio galaxies of the intracluster medium when harbored in galaxy clusters, as the case of G4Jy 1518 and G4Jy 1664; and (iii) detect X-ray radiation arising from their radio lobes, as for G4Jy 1863. |
publishDate |
2023 |
dc.date.none.fl_str_mv |
2023-09 |
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/11336/256408 Massaro, F.; White, S. V.; Paggi, A.; Jimenez Gallardo, A.; Madrid, J. P.; et al.; Powerful Radio Sources in the Southern Sky. II. A Swift X-Ray Perspective; IOP Publishing; Astrophysical Journal Supplement Series; 268; 1; 9-2023; 32-49 0067-0049 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/256408 |
identifier_str_mv |
Massaro, F.; White, S. V.; Paggi, A.; Jimenez Gallardo, A.; Madrid, J. P.; et al.; Powerful Radio Sources in the Southern Sky. II. A Swift X-Ray Perspective; IOP Publishing; Astrophysical Journal Supplement Series; 268; 1; 9-2023; 32-49 0067-0049 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4365/ace1f5 info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4365/ace1f5 |
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 |
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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1846083135777800192 |
score |
13.22299 |