Confirmation of a galaxy cluster hidden behind the Galactic bulge using the VVV survey

Autores
Coldwell Lloveras, Georgina Vanesa; Alonso Giraldes, Maria Sol; Duplancic Videla, Maria Fernanda; Hempel, Maren; Ivanov, Valentin D.; Minniti, Dante
Año de publicación
2014
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Context. S uzaku and Chandra X-ray observations detected a new cluster of galaxies, Suzaku J1759−3450, at a redshift z = 0.13. It is located behind the Milky Way, and the high Galactic dust extinction renders it nearly invisible at optical wavelengths. Aims. We attempt here to confirm the galaxy cluster with near-infrared imaging observations and to characterize its central member galaxies. Methods. Images from the VVV survey were used to detect candidate member galaxies of Suzaku J1759−3450 within the central region of the cluster up to 350 kpc from the X-ray peak emission. Color–magnitude diagrams, color–color diagrams, and morphology criteria allowed us to select the galaxies among the numerous foreground sources. Results. Fifteen candidate cluster members were found very close to a modeled red-sequence at the redshift of the cluster. Five members are extremely bright, and one is possibly a cD galaxy. The asymmetry in the spatial distribution of the galaxies with respect to the X-ray peak emission is an indicator that this cluster is still suffering a virialization process. Conclusions. Our investigation of Suzaku J1759−3450 demonstrates the potential of the VVV survey to study the hidden population of galaxies in the zone of avoidance.
Fil: Coldwell Lloveras, Georgina Vanesa. Universidad Nacional de San Juan. Facultad de Ciencias Exactas, Físicas y Naturales. Departamento de Geofísica y Astronomía; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan; Argentina
Fil: Alonso Giraldes, Maria Sol. Universidad Nacional de San Juan. Facultad de Ciencias Exactas, Físicas y Naturales. Departamento de Geofísica y Astronomía; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan; Argentina
Fil: Duplancic Videla, Maria Fernanda. Universidad Nacional de San Juan. Facultad de Ciencias Exactas, Físicas y Naturales. Departamento de Geofísica y Astronomía; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan; Argentina
Fil: Hempel, Maren. Pontificia Universidad Católica de Chile; Chile
Fil: Ivanov, Valentin D.. Observatorio Europeo del Sur; Chile
Fil: Minniti, Dante. Observatorio Europeo del Sur; Chile. Specola Vaticana Osservatorio Astronomico Vaticano; Italia. Universidad Andrés Bello; Chile
Materia
SURVEY
GALAXIES
BULGE
CLUSTER
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/155605
Acceder
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network_acronym_str CONICETDig
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network_name_str CONICET Digital (CONICET)
spelling Confirmation of a galaxy cluster hidden behind the Galactic bulge using the VVV surveyColdwell Lloveras, Georgina VanesaAlonso Giraldes, Maria SolDuplancic Videla, Maria FernandaHempel, MarenIvanov, Valentin D.Minniti, DanteSURVEYGALAXIESBULGECLUSTERhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Context. S uzaku and Chandra X-ray observations detected a new cluster of galaxies, Suzaku J1759−3450, at a redshift z = 0.13. It is located behind the Milky Way, and the high Galactic dust extinction renders it nearly invisible at optical wavelengths. Aims. We attempt here to confirm the galaxy cluster with near-infrared imaging observations and to characterize its central member galaxies. Methods. Images from the VVV survey were used to detect candidate member galaxies of Suzaku J1759−3450 within the central region of the cluster up to 350 kpc from the X-ray peak emission. Color–magnitude diagrams, color–color diagrams, and morphology criteria allowed us to select the galaxies among the numerous foreground sources. Results. Fifteen candidate cluster members were found very close to a modeled red-sequence at the redshift of the cluster. Five members are extremely bright, and one is possibly a cD galaxy. The asymmetry in the spatial distribution of the galaxies with respect to the X-ray peak emission is an indicator that this cluster is still suffering a virialization process. Conclusions. Our investigation of Suzaku J1759−3450 demonstrates the potential of the VVV survey to study the hidden population of galaxies in the zone of avoidance.Fil: Coldwell Lloveras, Georgina Vanesa. Universidad Nacional de San Juan. Facultad de Ciencias Exactas, Físicas y Naturales. Departamento de Geofísica y Astronomía; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan; ArgentinaFil: Alonso Giraldes, Maria Sol. Universidad Nacional de San Juan. Facultad de Ciencias Exactas, Físicas y Naturales. Departamento de Geofísica y Astronomía; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan; ArgentinaFil: Duplancic Videla, Maria Fernanda. Universidad Nacional de San Juan. Facultad de Ciencias Exactas, Físicas y Naturales. Departamento de Geofísica y Astronomía; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan; ArgentinaFil: Hempel, Maren. Pontificia Universidad Católica de Chile; ChileFil: Ivanov, Valentin D.. Observatorio Europeo del Sur; ChileFil: Minniti, Dante. Observatorio Europeo del Sur; Chile. Specola Vaticana Osservatorio Astronomico Vaticano; Italia. Universidad Andrés Bello; ChileEDP Sciences2014-09info: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/11336/155605Coldwell Lloveras, Georgina Vanesa; Alonso Giraldes, Maria Sol; Duplancic Videla, Maria Fernanda; Hempel, Maren; Ivanov, Valentin D.; et al.; Confirmation of a galaxy cluster hidden behind the Galactic bulge using the VVV survey; EDP Sciences; Astronomy and Astrophysics; 569; A49; 9-2014; 1-70004-6361CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/full_html/2014/09/aa23464-14/aa23464-14.htmlinfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201423464info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:10:41Zoai:ri.conicet.gov.ar:11336/155605instacron: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:34982025-10-22 11:10:41.315CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Confirmation of a galaxy cluster hidden behind the Galactic bulge using the VVV survey
title Confirmation of a galaxy cluster hidden behind the Galactic bulge using the VVV survey
spellingShingle Confirmation of a galaxy cluster hidden behind the Galactic bulge using the VVV survey
Coldwell Lloveras, Georgina Vanesa
SURVEY
GALAXIES
BULGE
CLUSTER
title_short Confirmation of a galaxy cluster hidden behind the Galactic bulge using the VVV survey
title_full Confirmation of a galaxy cluster hidden behind the Galactic bulge using the VVV survey
title_fullStr Confirmation of a galaxy cluster hidden behind the Galactic bulge using the VVV survey
title_full_unstemmed Confirmation of a galaxy cluster hidden behind the Galactic bulge using the VVV survey
title_sort Confirmation of a galaxy cluster hidden behind the Galactic bulge using the VVV survey
dc.creator.none.fl_str_mv Coldwell Lloveras, Georgina Vanesa
Alonso Giraldes, Maria Sol
Duplancic Videla, Maria Fernanda
Hempel, Maren
Ivanov, Valentin D.
Minniti, Dante
author Coldwell Lloveras, Georgina Vanesa
author_facet Coldwell Lloveras, Georgina Vanesa
Alonso Giraldes, Maria Sol
Duplancic Videla, Maria Fernanda
Hempel, Maren
Ivanov, Valentin D.
Minniti, Dante
author_role author
author2 Alonso Giraldes, Maria Sol
Duplancic Videla, Maria Fernanda
Hempel, Maren
Ivanov, Valentin D.
Minniti, Dante
author2_role author
author
author
author
author
dc.subject.none.fl_str_mv SURVEY
GALAXIES
BULGE
CLUSTER
topic SURVEY
GALAXIES
BULGE
CLUSTER
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. S uzaku and Chandra X-ray observations detected a new cluster of galaxies, Suzaku J1759−3450, at a redshift z = 0.13. It is located behind the Milky Way, and the high Galactic dust extinction renders it nearly invisible at optical wavelengths. Aims. We attempt here to confirm the galaxy cluster with near-infrared imaging observations and to characterize its central member galaxies. Methods. Images from the VVV survey were used to detect candidate member galaxies of Suzaku J1759−3450 within the central region of the cluster up to 350 kpc from the X-ray peak emission. Color–magnitude diagrams, color–color diagrams, and morphology criteria allowed us to select the galaxies among the numerous foreground sources. Results. Fifteen candidate cluster members were found very close to a modeled red-sequence at the redshift of the cluster. Five members are extremely bright, and one is possibly a cD galaxy. The asymmetry in the spatial distribution of the galaxies with respect to the X-ray peak emission is an indicator that this cluster is still suffering a virialization process. Conclusions. Our investigation of Suzaku J1759−3450 demonstrates the potential of the VVV survey to study the hidden population of galaxies in the zone of avoidance.
Fil: Coldwell Lloveras, Georgina Vanesa. Universidad Nacional de San Juan. Facultad de Ciencias Exactas, Físicas y Naturales. Departamento de Geofísica y Astronomía; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan; Argentina
Fil: Alonso Giraldes, Maria Sol. Universidad Nacional de San Juan. Facultad de Ciencias Exactas, Físicas y Naturales. Departamento de Geofísica y Astronomía; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan; Argentina
Fil: Duplancic Videla, Maria Fernanda. Universidad Nacional de San Juan. Facultad de Ciencias Exactas, Físicas y Naturales. Departamento de Geofísica y Astronomía; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan; Argentina
Fil: Hempel, Maren. Pontificia Universidad Católica de Chile; Chile
Fil: Ivanov, Valentin D.. Observatorio Europeo del Sur; Chile
Fil: Minniti, Dante. Observatorio Europeo del Sur; Chile. Specola Vaticana Osservatorio Astronomico Vaticano; Italia. Universidad Andrés Bello; Chile
description Context. S uzaku and Chandra X-ray observations detected a new cluster of galaxies, Suzaku J1759−3450, at a redshift z = 0.13. It is located behind the Milky Way, and the high Galactic dust extinction renders it nearly invisible at optical wavelengths. Aims. We attempt here to confirm the galaxy cluster with near-infrared imaging observations and to characterize its central member galaxies. Methods. Images from the VVV survey were used to detect candidate member galaxies of Suzaku J1759−3450 within the central region of the cluster up to 350 kpc from the X-ray peak emission. Color–magnitude diagrams, color–color diagrams, and morphology criteria allowed us to select the galaxies among the numerous foreground sources. Results. Fifteen candidate cluster members were found very close to a modeled red-sequence at the redshift of the cluster. Five members are extremely bright, and one is possibly a cD galaxy. The asymmetry in the spatial distribution of the galaxies with respect to the X-ray peak emission is an indicator that this cluster is still suffering a virialization process. Conclusions. Our investigation of Suzaku J1759−3450 demonstrates the potential of the VVV survey to study the hidden population of galaxies in the zone of avoidance.
publishDate 2014
dc.date.none.fl_str_mv 2014-09
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/11336/155605
Coldwell Lloveras, Georgina Vanesa; Alonso Giraldes, Maria Sol; Duplancic Videla, Maria Fernanda; Hempel, Maren; Ivanov, Valentin D.; et al.; Confirmation of a galaxy cluster hidden behind the Galactic bulge using the VVV survey; EDP Sciences; Astronomy and Astrophysics; 569; A49; 9-2014; 1-7
0004-6361
CONICET Digital
CONICET
url http://hdl.handle.net/11336/155605
identifier_str_mv Coldwell Lloveras, Georgina Vanesa; Alonso Giraldes, Maria Sol; Duplancic Videla, Maria Fernanda; Hempel, Maren; Ivanov, Valentin D.; et al.; Confirmation of a galaxy cluster hidden behind the Galactic bulge using the VVV survey; EDP Sciences; Astronomy and Astrophysics; 569; A49; 9-2014; 1-7
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/url/https://www.aanda.org/articles/aa/full_html/2014/09/aa23464-14/aa23464-14.html
info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201423464
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
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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score 12.982451

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