Powerful Radio Sources in the Southern Sky. I. Optical Identifications
- Autores
- Massaro, F.; White, S. V.; García Pérez, A.; Jimenez Gallardo, A.; Capetti, A.; Cheung, C. C.; Forman, W. R.; Mazzucchelli, C.; Paggi, A.; Nesvadba, N. P. H.; Madrid, J.P.; Andruchow, Ileana; Cellone, Sergio Aldo; Peña Herazo, H. A.; Grossová, R.; Balmaverde, B.; Sani, E.; Chavushyan, V.; Kraft, R. P.; Reynaldi, María Victoria; Leto, C.
- Año de publicación
- 2023
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Since the early sixties, our view of radio galaxies and quasars has been drastically shaped by discoveries made thanks to observations of radio sources listed in the Third Cambridge Catalog and its revised version (3CR). However, the largest fraction of data collected to date on 3CR sources was performed with relatively old instruments, rarely repeated and/or updated. Importantly, the 3CR contains only objects located in the Northern Hemisphere, thus having limited access to new and innovative astronomical facilities. To mitigate these limitations, we present a new catalog of powerful radio sources visible from the Southern Hemisphere, extracted from the GLEAM 4 Jy (G4Jy) catalog and based on equivalent selection criteria as the 3CR. This new catalog, named G4Jy-3CRE, where the E stands for “equivalent,” lists a total of 264 sources at decl. below −5° and with 9 Jy limiting sensitivity at ∼178 MHz. We explored archival radio maps obtained with different surveys and compared them with optical images available in the Pan-STARRS, DES, and DSS databases to search for optical counterparts of their radio cores. We compared mid-infrared counterparts, originally associated in the G4Jy, with the optical ones identified here, and we present results of a vast literature search carried out to collect redshift estimates for all G4Jy-3CRE sources resulting in a total of 145 reliable z measurements.
Fil: Massaro, F.. Università di Torino; Italia
Fil: White, S. V.. Rhodes University; Sudáfrica
Fil: García Pérez, A.. Università di Torino; Italia
Fil: Jimenez Gallardo, A.. Università di Torino; Italia
Fil: Capetti, A.. Osservatorio Astrofisico di Torino; Italia
Fil: Cheung, C. C.. Università di Torino; Italia
Fil: Forman, W. R.. No especifíca;
Fil: Mazzucchelli, C.. Universidad Diego Portales; Chile
Fil: Paggi, A.. Istituto Nazionale di Astrofisica; Italia
Fil: Nesvadba, N. P. H.. Universidad de Bologna; Italia
Fil: Madrid, J.P.. Istituto Nazionale di Astrofisica; Italia
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
Fil: Cellone, Sergio Aldo. Harvard-Smithsonian Center for Astrophysics; Estados Unidos. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; Argentina
Fil: Peña Herazo, H. A.. Masaryk University; República Checa
Fil: Grossová, R.. Universidad Diego Portales; Chile
Fil: Balmaverde, B.. Università di Torino; Italia
Fil: Sani, E.. No especifíca;
Fil: Chavushyan, V.. Istituto Nazionale di Astrofisica; Italia
Fil: Kraft, R. P.. No especifíca;
Fil: Reynaldi, María Victoria. 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: Leto, C.. No especifíca; - Materia
-
EXTRAGALACTIC RADIO SOURCES: 508
ASTROPHYSICS - ASTROPHYSICS OF GALAXIES
ASTROPHYSICS - HIGH ENERGY ASTROPHYSICAL PHENOMENA - 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:11336/256407
Ver los metadatos del registro completo
id |
CONICETDig_0dbdb653ec22f3f17da992e576d1aae4 |
---|---|
oai_identifier_str |
oai:ri.conicet.gov.ar:11336/256407 |
network_acronym_str |
CONICETDig |
repository_id_str |
3498 |
network_name_str |
CONICET Digital (CONICET) |
spelling |
Powerful Radio Sources in the Southern Sky. I. Optical IdentificationsMassaro, F.White, S. V.García Pérez, A.Jimenez Gallardo, A.Capetti, A.Cheung, C. C.Forman, W. R.Mazzucchelli, C.Paggi, A.Nesvadba, N. P. H.Madrid, J.P.Andruchow, IleanaCellone, Sergio AldoPeña Herazo, H. A.Grossová, R.Balmaverde, B.Sani, E.Chavushyan, V.Kraft, R. P.Reynaldi, María VictoriaLeto, C.EXTRAGALACTIC RADIO SOURCES: 508ASTROPHYSICS - ASTROPHYSICS OF GALAXIESASTROPHYSICS - HIGH ENERGY ASTROPHYSICAL PHENOMENAhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Since the early sixties, our view of radio galaxies and quasars has been drastically shaped by discoveries made thanks to observations of radio sources listed in the Third Cambridge Catalog and its revised version (3CR). However, the largest fraction of data collected to date on 3CR sources was performed with relatively old instruments, rarely repeated and/or updated. Importantly, the 3CR contains only objects located in the Northern Hemisphere, thus having limited access to new and innovative astronomical facilities. To mitigate these limitations, we present a new catalog of powerful radio sources visible from the Southern Hemisphere, extracted from the GLEAM 4 Jy (G4Jy) catalog and based on equivalent selection criteria as the 3CR. This new catalog, named G4Jy-3CRE, where the E stands for “equivalent,” lists a total of 264 sources at decl. below −5° and with 9 Jy limiting sensitivity at ∼178 MHz. We explored archival radio maps obtained with different surveys and compared them with optical images available in the Pan-STARRS, DES, and DSS databases to search for optical counterparts of their radio cores. We compared mid-infrared counterparts, originally associated in the G4Jy, with the optical ones identified here, and we present results of a vast literature search carried out to collect redshift estimates for all G4Jy-3CRE sources resulting in a total of 145 reliable z measurements.Fil: Massaro, F.. Università di Torino; ItaliaFil: White, S. V.. Rhodes University; SudáfricaFil: García Pérez, A.. Università di Torino; ItaliaFil: Jimenez Gallardo, A.. Università di Torino; ItaliaFil: Capetti, A.. Osservatorio Astrofisico di Torino; ItaliaFil: Cheung, C. C.. Università di Torino; ItaliaFil: Forman, W. R.. No especifíca;Fil: Mazzucchelli, C.. Universidad Diego Portales; ChileFil: Paggi, A.. Istituto Nazionale di Astrofisica; ItaliaFil: Nesvadba, N. P. H.. Universidad de Bologna; ItaliaFil: Madrid, J.P.. Istituto Nazionale di Astrofisica; ItaliaFil: 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; ArgentinaFil: Cellone, Sergio Aldo. Harvard-Smithsonian Center for Astrophysics; Estados Unidos. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; ArgentinaFil: Peña Herazo, H. A.. Masaryk University; República ChecaFil: Grossová, R.. Universidad Diego Portales; ChileFil: Balmaverde, B.. Università di Torino; ItaliaFil: Sani, E.. No especifíca;Fil: Chavushyan, V.. Istituto Nazionale di Astrofisica; ItaliaFil: Kraft, R. P.. No especifíca;Fil: Reynaldi, María Victoria. 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: Leto, C.. No especifíca;IOP Publishing2023-04info: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/11336/256407Massaro, F.; White, S. V.; García Pérez, A.; Jimenez Gallardo, A.; Capetti, A.; et al.; Powerful Radio Sources in the Southern Sky. I. Optical Identifications; IOP Publishing; Astrophysical Journal Supplement Series; 265; 2; 4-2023; 32-640067-0049CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4365/acaf05info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4365/acaf05info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-17T11:57:19Zoai:ri.conicet.gov.ar:11336/256407instacron: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:34982025-09-17 11:57:20.124CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Powerful Radio Sources in the Southern Sky. I. Optical Identifications |
title |
Powerful Radio Sources in the Southern Sky. I. Optical Identifications |
spellingShingle |
Powerful Radio Sources in the Southern Sky. I. Optical Identifications Massaro, F. EXTRAGALACTIC RADIO SOURCES: 508 ASTROPHYSICS - ASTROPHYSICS OF GALAXIES ASTROPHYSICS - HIGH ENERGY ASTROPHYSICAL PHENOMENA |
title_short |
Powerful Radio Sources in the Southern Sky. I. Optical Identifications |
title_full |
Powerful Radio Sources in the Southern Sky. I. Optical Identifications |
title_fullStr |
Powerful Radio Sources in the Southern Sky. I. Optical Identifications |
title_full_unstemmed |
Powerful Radio Sources in the Southern Sky. I. Optical Identifications |
title_sort |
Powerful Radio Sources in the Southern Sky. I. Optical Identifications |
dc.creator.none.fl_str_mv |
Massaro, F. White, S. V. García Pérez, A. Jimenez Gallardo, A. Capetti, A. Cheung, C. C. Forman, W. R. Mazzucchelli, C. Paggi, A. Nesvadba, N. P. H. Madrid, J.P. Andruchow, Ileana Cellone, Sergio Aldo Peña Herazo, H. A. Grossová, R. Balmaverde, B. Sani, E. Chavushyan, V. Kraft, R. P. Reynaldi, María Victoria Leto, C. |
author |
Massaro, F. |
author_facet |
Massaro, F. White, S. V. García Pérez, A. Jimenez Gallardo, A. Capetti, A. Cheung, C. C. Forman, W. R. Mazzucchelli, C. Paggi, A. Nesvadba, N. P. H. Madrid, J.P. Andruchow, Ileana Cellone, Sergio Aldo Peña Herazo, H. A. Grossová, R. Balmaverde, B. Sani, E. Chavushyan, V. Kraft, R. P. Reynaldi, María Victoria Leto, C. |
author_role |
author |
author2 |
White, S. V. García Pérez, A. Jimenez Gallardo, A. Capetti, A. Cheung, C. C. Forman, W. R. Mazzucchelli, C. Paggi, A. Nesvadba, N. P. H. Madrid, J.P. Andruchow, Ileana Cellone, Sergio Aldo Peña Herazo, H. A. Grossová, R. Balmaverde, B. Sani, E. Chavushyan, V. Kraft, R. P. Reynaldi, María Victoria Leto, C. |
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 |
EXTRAGALACTIC RADIO SOURCES: 508 ASTROPHYSICS - ASTROPHYSICS OF GALAXIES ASTROPHYSICS - HIGH ENERGY ASTROPHYSICAL PHENOMENA |
topic |
EXTRAGALACTIC RADIO SOURCES: 508 ASTROPHYSICS - ASTROPHYSICS OF GALAXIES ASTROPHYSICS - HIGH ENERGY ASTROPHYSICAL PHENOMENA |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
Since the early sixties, our view of radio galaxies and quasars has been drastically shaped by discoveries made thanks to observations of radio sources listed in the Third Cambridge Catalog and its revised version (3CR). However, the largest fraction of data collected to date on 3CR sources was performed with relatively old instruments, rarely repeated and/or updated. Importantly, the 3CR contains only objects located in the Northern Hemisphere, thus having limited access to new and innovative astronomical facilities. To mitigate these limitations, we present a new catalog of powerful radio sources visible from the Southern Hemisphere, extracted from the GLEAM 4 Jy (G4Jy) catalog and based on equivalent selection criteria as the 3CR. This new catalog, named G4Jy-3CRE, where the E stands for “equivalent,” lists a total of 264 sources at decl. below −5° and with 9 Jy limiting sensitivity at ∼178 MHz. We explored archival radio maps obtained with different surveys and compared them with optical images available in the Pan-STARRS, DES, and DSS databases to search for optical counterparts of their radio cores. We compared mid-infrared counterparts, originally associated in the G4Jy, with the optical ones identified here, and we present results of a vast literature search carried out to collect redshift estimates for all G4Jy-3CRE sources resulting in a total of 145 reliable z measurements. Fil: Massaro, F.. Università di Torino; Italia Fil: White, S. V.. Rhodes University; Sudáfrica Fil: García Pérez, A.. Università di Torino; Italia Fil: Jimenez Gallardo, A.. Università di Torino; Italia Fil: Capetti, A.. Osservatorio Astrofisico di Torino; Italia Fil: Cheung, C. C.. Università di Torino; Italia Fil: Forman, W. R.. No especifíca; Fil: Mazzucchelli, C.. Universidad Diego Portales; Chile Fil: Paggi, A.. Istituto Nazionale di Astrofisica; Italia Fil: Nesvadba, N. P. H.. Universidad de Bologna; Italia Fil: Madrid, J.P.. Istituto Nazionale di Astrofisica; Italia 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 Fil: Cellone, Sergio Aldo. Harvard-Smithsonian Center for Astrophysics; Estados Unidos. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; Argentina Fil: Peña Herazo, H. A.. Masaryk University; República Checa Fil: Grossová, R.. Universidad Diego Portales; Chile Fil: Balmaverde, B.. Università di Torino; Italia Fil: Sani, E.. No especifíca; Fil: Chavushyan, V.. Istituto Nazionale di Astrofisica; Italia Fil: Kraft, R. P.. No especifíca; Fil: Reynaldi, María Victoria. 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: Leto, C.. No especifíca; |
description |
Since the early sixties, our view of radio galaxies and quasars has been drastically shaped by discoveries made thanks to observations of radio sources listed in the Third Cambridge Catalog and its revised version (3CR). However, the largest fraction of data collected to date on 3CR sources was performed with relatively old instruments, rarely repeated and/or updated. Importantly, the 3CR contains only objects located in the Northern Hemisphere, thus having limited access to new and innovative astronomical facilities. To mitigate these limitations, we present a new catalog of powerful radio sources visible from the Southern Hemisphere, extracted from the GLEAM 4 Jy (G4Jy) catalog and based on equivalent selection criteria as the 3CR. This new catalog, named G4Jy-3CRE, where the E stands for “equivalent,” lists a total of 264 sources at decl. below −5° and with 9 Jy limiting sensitivity at ∼178 MHz. We explored archival radio maps obtained with different surveys and compared them with optical images available in the Pan-STARRS, DES, and DSS databases to search for optical counterparts of their radio cores. We compared mid-infrared counterparts, originally associated in the G4Jy, with the optical ones identified here, and we present results of a vast literature search carried out to collect redshift estimates for all G4Jy-3CRE sources resulting in a total of 145 reliable z measurements. |
publishDate |
2023 |
dc.date.none.fl_str_mv |
2023-04 |
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/11336/256407 Massaro, F.; White, S. V.; García Pérez, A.; Jimenez Gallardo, A.; Capetti, A.; et al.; Powerful Radio Sources in the Southern Sky. I. Optical Identifications; IOP Publishing; Astrophysical Journal Supplement Series; 265; 2; 4-2023; 32-64 0067-0049 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/256407 |
identifier_str_mv |
Massaro, F.; White, S. V.; García Pérez, A.; Jimenez Gallardo, A.; Capetti, A.; et al.; Powerful Radio Sources in the Southern Sky. I. Optical Identifications; IOP Publishing; Astrophysical Journal Supplement Series; 265; 2; 4-2023; 32-64 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/acaf05 info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4365/acaf05 |
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 |
_version_ |
1843606916631101440 |
score |
13.001348 |