Ultracool dwarfs in deep extragalactic surveys using the virtual observatory: ALHAMBRA and COSMOS

This article is published and distributed under the terms of the Oxford University Press, Standard Journals Publication Model (https://academic.oup.com/journals/pages/open_access/funder_policies/chorus/standard_publication_model)

Detalles Bibliográficos
Autores: Solano, Enrique, Gálvez Ortiz, M. C., Martín, Eduardo L., Gómez Muñoz, I. M., Rodrigo, C., Burgasser, A. J., Lodieu, N., Béjar, V. J. S., Huélamo, N., Morales Calderón, M., Bouy, H.
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2021
País:España
Institución:Instituto Nacional de Técnica Aeroespacial (INTA)
Repositorio:DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
OAI Identifier:oai:digital.inta.es:20.500.12666/565
Acceso en línea:https://academic.oup.com/mnras/article-abstract/501/1/281/6039331
http://hdl.handle.net/20.500.12666/565
Access Level:acceso abierto
Palabra clave:Surveys
Virtual observatory tools
Brown dwarfs
Stars: low mass
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oai_identifier_str oai:digital.inta.es:20.500.12666/565
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repository_id_str
dc.title.none.fl_str_mv Ultracool dwarfs in deep extragalactic surveys using the virtual observatory: ALHAMBRA and COSMOS
title Ultracool dwarfs in deep extragalactic surveys using the virtual observatory: ALHAMBRA and COSMOS
spellingShingle Ultracool dwarfs in deep extragalactic surveys using the virtual observatory: ALHAMBRA and COSMOS
Solano, Enrique
Surveys
Virtual observatory tools
Brown dwarfs
Stars: low mass
title_short Ultracool dwarfs in deep extragalactic surveys using the virtual observatory: ALHAMBRA and COSMOS
title_full Ultracool dwarfs in deep extragalactic surveys using the virtual observatory: ALHAMBRA and COSMOS
title_fullStr Ultracool dwarfs in deep extragalactic surveys using the virtual observatory: ALHAMBRA and COSMOS
title_full_unstemmed Ultracool dwarfs in deep extragalactic surveys using the virtual observatory: ALHAMBRA and COSMOS
title_sort Ultracool dwarfs in deep extragalactic surveys using the virtual observatory: ALHAMBRA and COSMOS
dc.creator.none.fl_str_mv Solano, Enrique
Gálvez Ortiz, M. C.
Martín, Eduardo L.
Gómez Muñoz, I. M.
Rodrigo, C.
Burgasser, A. J.
Lodieu, N.
Béjar, V. J. S.
Huélamo, N.
Morales Calderón, M.
Bouy, H.
author Solano, Enrique
author_facet Solano, Enrique
Gálvez Ortiz, M. C.
Martín, Eduardo L.
Gómez Muñoz, I. M.
Rodrigo, C.
Burgasser, A. J.
Lodieu, N.
Béjar, V. J. S.
Huélamo, N.
Morales Calderón, M.
Bouy, H.
author_role author
author2 Gálvez Ortiz, M. C.
Martín, Eduardo L.
Gómez Muñoz, I. M.
Rodrigo, C.
Burgasser, A. J.
Lodieu, N.
Béjar, V. J. S.
Huélamo, N.
Morales Calderón, M.
Bouy, H.
author2_role author
author
author
author
author
author
author
author
author
author
dc.contributor.none.fl_str_mv Unidad de Excelencia Científica María de Maeztu Centro de Astrobiología del Instituto Nacional de Técnica Aeroespacial y CSIC, MDM-2017-0737
Agencia Estatal de Investigación (AEI)
Ministerio de Economía y Competitividad (MINECO)
dc.subject.none.fl_str_mv Surveys
Virtual observatory tools
Brown dwarfs
Stars: low mass
topic Surveys
Virtual observatory tools
Brown dwarfs
Stars: low mass
description This article is published and distributed under the terms of the Oxford University Press, Standard Journals Publication Model (https://academic.oup.com/journals/pages/open_access/funder_policies/chorus/standard_publication_model)
publishDate 2021
dc.date.none.fl_str_mv 2021
2022
2022
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv https://academic.oup.com/mnras/article-abstract/501/1/281/6039331
http://hdl.handle.net/20.500.12666/565
url https://academic.oup.com/mnras/article-abstract/501/1/281/6039331
http://hdl.handle.net/20.500.12666/565
dc.language.none.fl_str_mv Inglés
language_invalid_str_mv Inglés
dc.relation.none.fl_str_mv EL OBSERVATORIO VIRTUAL ESPAÑOL. EXPLOTACION CIENTIFICO-TECNICA DE ARCHIVOS ASTRONOMICOS
info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/AYA2017-84089-P
ENANAS ULTRAFRIAS: UN ESLABON UNICO ENTRE ESTRELLAS Y PLANETAS
ORIGEN Y EVOLUCION DE LAS ENANAS MARRONES Y PLANETAS GIGANTES
info:eu-repo/grantAgreement/MINECO//AYA2015-69350-C3-1-P
info:eu-repo/grantAgreement/MINECO//AYA2015-69350-C3-2-P
dc.rights.none.fl_str_mv Attribution 4.0 International
https://creativecommons.org/licenses/by/4.0/
info:eu-repo/semantics/openAccess
rights_invalid_str_mv Attribution 4.0 International
https://creativecommons.org/licenses/by/4.0/
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv Oxford Academics: Oxford University Press
publisher.none.fl_str_mv Oxford Academics: Oxford University Press
dc.source.none.fl_str_mv reponame:DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
instname:Instituto Nacional de Técnica Aeroespacial (INTA)
instname_str Instituto Nacional de Técnica Aeroespacial (INTA)
reponame_str DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
collection DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
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spelling Ultracool dwarfs in deep extragalactic surveys using the virtual observatory: ALHAMBRA and COSMOSSolano, EnriqueGálvez Ortiz, M. C.Martín, Eduardo L.Gómez Muñoz, I. M.Rodrigo, C.Burgasser, A. J.Lodieu, N.Béjar, V. J. S.Huélamo, N.Morales Calderón, M.Bouy, H.SurveysVirtual observatory toolsBrown dwarfsStars: low massThis article is published and distributed under the terms of the Oxford University Press, Standard Journals Publication Model (https://academic.oup.com/journals/pages/open_access/funder_policies/chorus/standard_publication_model)Ultracool dwarfs (UCDs) encompass a wide variety of compact stellar-like objects with spectra classified as late-M, L, T, and Y. Most of them have been discovered using wide-field imaging surveys. The Virtual Observatory (VO) has proven to be of great utility to efficiently exploit these astronomical resources. We aim to validate a VO methodology designed to discover and characterize UCDs in deep extragalactic surveys like Advance Large Homogeneous Area Medium-Band Redshift Astronomical (ALHAMBRA) and Cosmological Evolution Survey (COSMOS). Three complimentary searches based on parallaxes, proper motions and colours, respectively, were carried out. A total of 897 candidate UCDs were found, with only 16 previously reported in SIMBAD. Most of the new UCDs reported here are likely late-M and L dwarfs because of the limitations imposed by the utilization of optical (Gaia DR2 and r-band) data. We complement ALHAMBRA and COSMOS photometry with other catalogues in the optical and infrared using VOSA, a VO tool that estimates effective temperatures from the spectral energy distribution fitting to collections of theoretical models. The agreement between the number of UCDs found in the COSMOS field and theoretical estimations together with the low false-negative rate (known UCDs not discovered in our search) validates the methodology proposed in this work, which will be used in the forthcoming wide and deep surveys provided by the Euclid space mission. Simulations of Euclid number counts for UCDs detectable in different photometric passbands are presented for a wide survey area of 15 000 deg2, and the limitations of applicability of Euclid data to detect UCDs using the methods employed in this paper are discussed.This research has made use of the Aladin sky atlas developed at CDS, Strasbourg Observatory, France. This publication makes use of VOSA, developed under the Spanish Virtual Observatory project supported from the Spanish MICIU through grant AyA2017-84089. This research has been partly funded by the Spanish State Research Agency (AEI) Project MDM-2017-0737 at Centro de Astrobiologia (CSIC-INTA), Unidad de Excelencia Maria de Maeztu. EM was supported by grant AYA2015-69350-C3-1-P. NL was supported by grant AYA2015-69350-C3-2-P. This work has made use of data from the European Space Agency (ESA) mission Gaia,13 processed by the Gaia Data Processing and Analysis Consortium (DPAC).14 We also extensivelymade use of TOPCAT (Taylor 2005) and STILTS (Taylor 2006) as well as the Vizier and SIMBAD services, both operated at CDS, Strasbourg, France.PeerreviewOxford Academics: Oxford University PressUnidad de Excelencia Científica María de Maeztu Centro de Astrobiología del Instituto Nacional de Técnica Aeroespacial y CSIC, MDM-2017-0737Agencia Estatal de Investigación (AEI)Ministerio de Economía y Competitividad (MINECO)202220222021info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501application/pdfhttps://academic.oup.com/mnras/article-abstract/501/1/281/6039331http://hdl.handle.net/20.500.12666/565reponame:DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacialinstname:Instituto Nacional de Técnica Aeroespacial (INTA)InglésEL OBSERVATORIO VIRTUAL ESPAÑOL. EXPLOTACION CIENTIFICO-TECNICA DE ARCHIVOS ASTRONOMICOSinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/AYA2017-84089-PENANAS ULTRAFRIAS: UN ESLABON UNICO ENTRE ESTRELLAS Y PLANETASORIGEN Y EVOLUCION DE LAS ENANAS MARRONES Y PLANETAS GIGANTESinfo:eu-repo/grantAgreement/MINECO//AYA2015-69350-C3-1-Pinfo:eu-repo/grantAgreement/MINECO//AYA2015-69350-C3-2-PAttribution 4.0 InternationalCopyright © 2020, © 2020 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Societyhttps://creativecommons.org/licenses/by/4.0/info:eu-repo/semantics/openAccessoai:digital.inta.es:20.500.12666/5652026-06-23T12:46:37Z
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