Powerful Radio Sources in the Southern Sky. II. A Swift X-Ray Perspective
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). Th...
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IOP Publishing
2023-01-01
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Online Access: | https://doi.org/10.3847/1538-4365/ace1f5 |
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author | F. Massaro S. V. White A. Paggi A. Jimenez-Gallardo J. P. Madrid C. Mazzucchelli W. R. Forman A. Capetti C. Leto A. García-Pérez C. C. Cheung V. Chavushyan N. P. H. Nesvadba I. Andruchow H. A. Peña-Herazo E. Sani R. Grossová V. Reynaldi R. P. Kraft B. Balmaverde S. Cellone |
author_facet | F. Massaro S. V. White A. Paggi A. Jimenez-Gallardo J. P. Madrid C. Mazzucchelli W. R. Forman A. Capetti C. Leto A. García-Pérez C. C. Cheung V. Chavushyan N. P. H. Nesvadba I. Andruchow H. A. Peña-Herazo E. Sani R. Grossová V. Reynaldi R. P. Kraft B. Balmaverde S. Cellone |
author_sort | F. Massaro |
collection | DOAJ |
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. |
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issn | 0067-0049 |
language | English |
last_indexed | 2024-03-12T02:02:55Z |
publishDate | 2023-01-01 |
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series | The Astrophysical Journal Supplement Series |
spelling | doaj.art-1859a01fb9784dffb3d653df94e948202023-09-07T08:59:03ZengIOP PublishingThe Astrophysical Journal Supplement Series0067-00492023-01-0126813210.3847/1538-4365/ace1f5Powerful Radio Sources in the Southern Sky. II. A Swift X-Ray PerspectiveF. Massaro0https://orcid.org/0000-0002-1704-9850S. V. White1https://orcid.org/0000-0002-2340-8303A. Paggi2https://orcid.org/0000-0002-5646-2410A. Jimenez-Gallardo3https://orcid.org/0000-0003-4413-7722J. P. Madrid4C. Mazzucchelli5https://orcid.org/0000-0002-5941-5214W. R. Forman6https://orcid.org/0000-0002-9478-1682A. Capetti7https://orcid.org/0000-0003-3684-4275C. Leto8A. García-Pérez9https://orcid.org/0000-0002-9896-6430C. C. Cheung10https://orcid.org/0000-0002-4377-0174V. Chavushyan11https://orcid.org/0000-0002-2558-0967N. P. H. Nesvadba12https://orcid.org/0000-0001-5783-6544I. Andruchow13https://orcid.org/0000-0003-1562-5188H. A. Peña-Herazo14https://orcid.org/0000-0003-0032-9538E. Sani15https://orcid.org/0000-0002-3140-4070R. Grossová16https://orcid.org/0000-0003-3471-7459V. Reynaldi17https://orcid.org/0000-0002-6472-6711R. P. Kraft18https://orcid.org/0000-0002-0765-0511B. Balmaverde19https://orcid.org/0000-0002-0690-0638S. Cellone20https://orcid.org/0000-0002-3866-2726Dipartimento di Fisica, Università degli Studi di Torino , via Pietro Giuria 1, I-10125 Torino, Italy ; f.massaro@unito.it; Istituto Nazionale di Astrofisica (INAF)— Osservatorio Astrofisico di Torino , via Osservatorio 20, I-10025 Pino Torinese, Italy; Istituto Nazionale di Fisica Nucleare (INFN)— Sezione di Torino , via Pietro Giuria 1, I-10125 Torino, Italy; Consorzio Interuniversitario per la Fisica Spaziale , via Pietro Giuria 1, I-10125 Torino, ItalyDepartment of Physics and Electronics, Rhodes University , P.O. Box 94, Grahamstown 6140, South AfricaDipartimento di Fisica, Università degli Studi di Torino (UniTO) , via Pietro Giuria 1, I-10125 Torino, Italy; Istituto Nazionale di Astrofisica—Osservatorio Astrofisico di Torino , via Osservatorio 20, I-10025 Pino Torinese, Italy; Istituto Nazionale di Fisica Nucleare—Sezione di Torino , via Pietro Giuria 1, I-10125 Torino, ItalyDipartimento di Fisica, Università degli Studi di Torino , via Pietro Giuria 1, I-10125 Torino, Italy ; f.massaro@unito.it; Istituto Nazionale di Astrofisica (INAF)— Osservatorio Astrofisico di Torino , via Osservatorio 20, I-10025 Pino Torinese, Italy; Dipartimento di Fisica e Astronomia, Università di Bologna , via P. Gobetti 93/2, I-40129 Bologna, ItalyDepartment of Physics and Astronomy, The University of Texas Rio Grande Valley , Brownsville, TX 78520, USAEuropean Southern Observatory , Alonso de Córdova 3107, Vitacura, Región Metropolitana, Chile; Instituto de Estudios Astrofísicos , Facultad de Ingeniería y Ciencias, Universidad Diego Portales, Avenida Ejercito Libertador 441, Santiago, ChileCenter for Astrophysics, Harvard & Smithsonian , 60 Garden Street, Cambridge, MA 02138, USAIstituto Nazionale di Astrofisica (INAF)— Osservatorio Astrofisico di Torino , via Osservatorio 20, I-10025 Pino Torinese, ItalyASI—Agenzia Spaziale Italiana , Via del Politecnico snc, I-00133 Roma, ItalyDipartimento di Fisica, Università degli Studi di Torino , via Pietro Giuria 1, I-10125 Torino, Italy ; f.massaro@unito.it; Instituto Nacional de Astrofísica , Óptica y Electrónica, Luis Enrique Erro 1, Tonantzintla, Puebla 72840, MéxicoSpace Science Division, Naval Research Laboratory , Washington, DC 20375, USACenter for Astrophysics, Harvard & Smithsonian , 60 Garden Street, Cambridge, MA 02138, USA; Instituto Nacional de Astrofísica , Óptica y Electrónica, Luis Enrique Erro 1, Tonantzintla, Puebla 72840, MéxicoUniversité de la Côte d’Azur , Observatoire de la Côte d’Azur, CNRS, Laboratoire Lagrange, Bd de l’Observatoire, CS 34229, F-06304 Nice cedex 4, FranceInstituto Argentino de Radioastronomía , CONICET-CICPBA-UNLP, CC5 (1897) Villa Elisa, Prov. de Buenos Aires, Argentina; Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de La Plata , Paseo del Bosque, B1900FWA La Plata, ArgentinaEast Asian Observatory , 660 N. A’ohōkū Place, Hilo, HI 96720, USAEuropean Southern Observatory , Alonso de Córdova 3107, Vitacura, Región Metropolitana, ChileDepartment of Theoretical Physics and Astrophysics, Faculty of Science, Masaryk University , Kotlářská 2, Brno CZ-611 37, Czech Republic; Astronomical Institute of the Czech Academy of Sciences , Bocní II 1401, 141 00 Prague, Czech RepublicFacultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de La Plata , Paseo del Bosque, B1900FWA La Plata, Argentina; Instituto de Astrofísica de La Plata (CCT La Plata-CONICET-UNLP) , La Plata, ArgentinaCenter for Astrophysics, Harvard & Smithsonian , 60 Garden Street, Cambridge, MA 02138, USAIstituto Nazionale di Astrofisica—Osservatorio Astrofisico di Torino , via Osservatorio 20, I-10025 Pino Torinese, ItalyFacultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de La Plata , Paseo del Bosque, B1900FWA La Plata, Argentina; Complejo Astronómico El Leoncito (CASLEO) , CONICET-UNLP-UNC-UNSJ, Av. España 1512 (sur), J5402DSP San Juan, ArgentinaWe 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.https://doi.org/10.3847/1538-4365/ace1f5Radio active galactic nucleiRadio jetsRadio lobesRadio loud quasarsGalaxy clustersGalactic and extragalactic astronomy |
spellingShingle | F. Massaro S. V. White A. Paggi A. Jimenez-Gallardo J. P. Madrid C. Mazzucchelli W. R. Forman A. Capetti C. Leto A. García-Pérez C. C. Cheung V. Chavushyan N. P. H. Nesvadba I. Andruchow H. A. Peña-Herazo E. Sani R. Grossová V. Reynaldi R. P. Kraft B. Balmaverde S. Cellone Powerful Radio Sources in the Southern Sky. II. A Swift X-Ray Perspective The Astrophysical Journal Supplement Series Radio active galactic nuclei Radio jets Radio lobes Radio loud quasars Galaxy clusters Galactic and extragalactic astronomy |
title | 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_short | 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 |
topic | Radio active galactic nuclei Radio jets Radio lobes Radio loud quasars Galaxy clusters Galactic and extragalactic astronomy |
url | https://doi.org/10.3847/1538-4365/ace1f5 |
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