Galaxies behind the galactic plane: First results and perspectives from the VVV survey
- Autores
- Amôres, E. B.; Sodré, Laerte; Minniti, D.; Alonso, Maria Victoria; Padilla, Nelson David; Gurovich, Sebastian; Arsenijevic, V.; Tollerud, E. J.; Rodríguez Ardila, A.; Diaz Tello, Jorge Andres; Lucas, P. W.
- Año de publicación
- 2012
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- VISTA Variables in the Via Láctea (VVV) is an ESO variability survey that is performing observations in near-infrared bands (ZY JHK s) toward the Galactic bulge and part of the disk with the completeness limits at least 3mag deeper than Two Micron All Sky Survey. In the present work, we searched in the VVV survey data for background galaxies near the Galactic plane using ZY JHK s photometry that covers 1.636deg2. We identified 204 new galaxy candidates by analyzing colors, sizes, and visual inspection of multi-band (ZY JHK s) images. The galaxy candidate colors were also compared with the predicted ones by star count models considering a more realistic extinction model at the same completeness limits observed by VVV. A comparison of the galaxy candidates with the expected one by Millennium simulations is also presented. Our results increase the number density of known galaxies behind the Milky Way by more than one order of magnitude. A catalog with galaxy properties including ellipticity, Petrosian radii, and ZY JHK s magnitudes is provided, as well as comparisons of the results with other surveys of galaxies toward the Galactic plane. © © 2012. The American Astronomical Society. All rights reserved..
Fil: Amôres, E. B.. Laboratorio Nacional de Astrofisica de Itajuba; Brasil. Universidade de Lisboa. Facultad de Ciencias; Portugal
Fil: Sodré, Laerte. Universidade do Sao Paulo. Instituto de Astronomia, Geofísica e Ciências Atmosféricas; Brasil
Fil: Minniti, D.. Pontificia Universidad Católica de Chile; Chile
Fil: Alonso, Maria Victoria. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Padilla, Nelson David. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Gurovich, Sebastian. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Arsenijevic, V.. Unversidad de Lisboa. Facultad de Ciencias; Portugal
Fil: Tollerud, E. J.. University of California at Irvine; Estados Unidos
Fil: Rodríguez Ardila, A.. Laboratorio Nacional de Astrofisica de Itajuba; Brasil
Fil: Diaz Tello, Jorge Andres. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Lucas, P. W.. University of Hertfordshire; Reino Unido - Materia
-
GALAXIES: FUNDAMENTAL PARAMETERS
GALAXIES: GENERAL
GALAXY: STRUCTURE
ISM: STRUCTURE
SURVEYS - 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:11336/190939
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Galaxies behind the galactic plane: First results and perspectives from the VVV surveyAmôres, E. B.Sodré, LaerteMinniti, D.Alonso, Maria VictoriaPadilla, Nelson DavidGurovich, SebastianArsenijevic, V.Tollerud, E. J.Rodríguez Ardila, A.Diaz Tello, Jorge AndresLucas, P. W.GALAXIES: FUNDAMENTAL PARAMETERSGALAXIES: GENERALGALAXY: STRUCTUREISM: STRUCTURESURVEYShttps://purl.org/becyt/ford/1.7https://purl.org/becyt/ford/1VISTA Variables in the Via Láctea (VVV) is an ESO variability survey that is performing observations in near-infrared bands (ZY JHK s) toward the Galactic bulge and part of the disk with the completeness limits at least 3mag deeper than Two Micron All Sky Survey. In the present work, we searched in the VVV survey data for background galaxies near the Galactic plane using ZY JHK s photometry that covers 1.636deg2. We identified 204 new galaxy candidates by analyzing colors, sizes, and visual inspection of multi-band (ZY JHK s) images. The galaxy candidate colors were also compared with the predicted ones by star count models considering a more realistic extinction model at the same completeness limits observed by VVV. A comparison of the galaxy candidates with the expected one by Millennium simulations is also presented. Our results increase the number density of known galaxies behind the Milky Way by more than one order of magnitude. A catalog with galaxy properties including ellipticity, Petrosian radii, and ZY JHK s magnitudes is provided, as well as comparisons of the results with other surveys of galaxies toward the Galactic plane. © © 2012. The American Astronomical Society. All rights reserved..Fil: Amôres, E. B.. Laboratorio Nacional de Astrofisica de Itajuba; Brasil. Universidade de Lisboa. Facultad de Ciencias; PortugalFil: Sodré, Laerte. Universidade do Sao Paulo. Instituto de Astronomia, Geofísica e Ciências Atmosféricas; BrasilFil: Minniti, D.. Pontificia Universidad Católica de Chile; ChileFil: Alonso, Maria Victoria. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaFil: Padilla, Nelson David. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Gurovich, Sebastian. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaFil: Arsenijevic, V.. Unversidad de Lisboa. Facultad de Ciencias; PortugalFil: Tollerud, E. J.. University of California at Irvine; Estados UnidosFil: Rodríguez Ardila, A.. Laboratorio Nacional de Astrofisica de Itajuba; BrasilFil: Diaz Tello, Jorge Andres. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaFil: Lucas, P. W.. University of Hertfordshire; Reino UnidoIOP Publishing2012-09-27info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/190939Amôres, E. B.; Sodré, Laerte; Minniti, D.; Alonso, Maria Victoria; Padilla, Nelson David; et al.; Galaxies behind the galactic plane: First results and perspectives from the VVV survey; IOP Publishing; Astronomical Journal; 144; 5; 27-9-20120004-62561538-3881CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1088/0004-6256/144/5/127info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1088/0004-6256/144/5/127info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:43:35Zoai:ri.conicet.gov.ar:11336/190939instacron: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 11:43:36.057CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Galaxies behind the galactic plane: First results and perspectives from the VVV survey |
title |
Galaxies behind the galactic plane: First results and perspectives from the VVV survey |
spellingShingle |
Galaxies behind the galactic plane: First results and perspectives from the VVV survey Amôres, E. B. GALAXIES: FUNDAMENTAL PARAMETERS GALAXIES: GENERAL GALAXY: STRUCTURE ISM: STRUCTURE SURVEYS |
title_short |
Galaxies behind the galactic plane: First results and perspectives from the VVV survey |
title_full |
Galaxies behind the galactic plane: First results and perspectives from the VVV survey |
title_fullStr |
Galaxies behind the galactic plane: First results and perspectives from the VVV survey |
title_full_unstemmed |
Galaxies behind the galactic plane: First results and perspectives from the VVV survey |
title_sort |
Galaxies behind the galactic plane: First results and perspectives from the VVV survey |
dc.creator.none.fl_str_mv |
Amôres, E. B. Sodré, Laerte Minniti, D. Alonso, Maria Victoria Padilla, Nelson David Gurovich, Sebastian Arsenijevic, V. Tollerud, E. J. Rodríguez Ardila, A. Diaz Tello, Jorge Andres Lucas, P. W. |
author |
Amôres, E. B. |
author_facet |
Amôres, E. B. Sodré, Laerte Minniti, D. Alonso, Maria Victoria Padilla, Nelson David Gurovich, Sebastian Arsenijevic, V. Tollerud, E. J. Rodríguez Ardila, A. Diaz Tello, Jorge Andres Lucas, P. W. |
author_role |
author |
author2 |
Sodré, Laerte Minniti, D. Alonso, Maria Victoria Padilla, Nelson David Gurovich, Sebastian Arsenijevic, V. Tollerud, E. J. Rodríguez Ardila, A. Diaz Tello, Jorge Andres Lucas, P. W. |
author2_role |
author author author author author author author author author author |
dc.subject.none.fl_str_mv |
GALAXIES: FUNDAMENTAL PARAMETERS GALAXIES: GENERAL GALAXY: STRUCTURE ISM: STRUCTURE SURVEYS |
topic |
GALAXIES: FUNDAMENTAL PARAMETERS GALAXIES: GENERAL GALAXY: STRUCTURE ISM: STRUCTURE SURVEYS |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.7 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
VISTA Variables in the Via Láctea (VVV) is an ESO variability survey that is performing observations in near-infrared bands (ZY JHK s) toward the Galactic bulge and part of the disk with the completeness limits at least 3mag deeper than Two Micron All Sky Survey. In the present work, we searched in the VVV survey data for background galaxies near the Galactic plane using ZY JHK s photometry that covers 1.636deg2. We identified 204 new galaxy candidates by analyzing colors, sizes, and visual inspection of multi-band (ZY JHK s) images. The galaxy candidate colors were also compared with the predicted ones by star count models considering a more realistic extinction model at the same completeness limits observed by VVV. A comparison of the galaxy candidates with the expected one by Millennium simulations is also presented. Our results increase the number density of known galaxies behind the Milky Way by more than one order of magnitude. A catalog with galaxy properties including ellipticity, Petrosian radii, and ZY JHK s magnitudes is provided, as well as comparisons of the results with other surveys of galaxies toward the Galactic plane. © © 2012. The American Astronomical Society. All rights reserved.. Fil: Amôres, E. B.. Laboratorio Nacional de Astrofisica de Itajuba; Brasil. Universidade de Lisboa. Facultad de Ciencias; Portugal Fil: Sodré, Laerte. Universidade do Sao Paulo. Instituto de Astronomia, Geofísica e Ciências Atmosféricas; Brasil Fil: Minniti, D.. Pontificia Universidad Católica de Chile; Chile Fil: Alonso, Maria Victoria. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina Fil: Padilla, Nelson David. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina Fil: Gurovich, Sebastian. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina Fil: Arsenijevic, V.. Unversidad de Lisboa. Facultad de Ciencias; Portugal Fil: Tollerud, E. J.. University of California at Irvine; Estados Unidos Fil: Rodríguez Ardila, A.. Laboratorio Nacional de Astrofisica de Itajuba; Brasil Fil: Diaz Tello, Jorge Andres. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina Fil: Lucas, P. W.. University of Hertfordshire; Reino Unido |
description |
VISTA Variables in the Via Láctea (VVV) is an ESO variability survey that is performing observations in near-infrared bands (ZY JHK s) toward the Galactic bulge and part of the disk with the completeness limits at least 3mag deeper than Two Micron All Sky Survey. In the present work, we searched in the VVV survey data for background galaxies near the Galactic plane using ZY JHK s photometry that covers 1.636deg2. We identified 204 new galaxy candidates by analyzing colors, sizes, and visual inspection of multi-band (ZY JHK s) images. The galaxy candidate colors were also compared with the predicted ones by star count models considering a more realistic extinction model at the same completeness limits observed by VVV. A comparison of the galaxy candidates with the expected one by Millennium simulations is also presented. Our results increase the number density of known galaxies behind the Milky Way by more than one order of magnitude. A catalog with galaxy properties including ellipticity, Petrosian radii, and ZY JHK s magnitudes is provided, as well as comparisons of the results with other surveys of galaxies toward the Galactic plane. © © 2012. The American Astronomical Society. All rights reserved.. |
publishDate |
2012 |
dc.date.none.fl_str_mv |
2012-09-27 |
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/11336/190939 Amôres, E. B.; Sodré, Laerte; Minniti, D.; Alonso, Maria Victoria; Padilla, Nelson David; et al.; Galaxies behind the galactic plane: First results and perspectives from the VVV survey; IOP Publishing; Astronomical Journal; 144; 5; 27-9-2012 0004-6256 1538-3881 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/190939 |
identifier_str_mv |
Amôres, E. B.; Sodré, Laerte; Minniti, D.; Alonso, Maria Victoria; Padilla, Nelson David; et al.; Galaxies behind the galactic plane: First results and perspectives from the VVV survey; IOP Publishing; Astronomical Journal; 144; 5; 27-9-2012 0004-6256 1538-3881 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1088/0004-6256/144/5/127 info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1088/0004-6256/144/5/127 |
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 |
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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12.982451 |