The GALANTE photometric system

This paper describes the characterization of the GALANTE photometric system, a seven intermediate-and narrow-band filter system with a wavelength coverage from 3000 Å to 9000 Å. We describe the photometric system presenting the full sensitivity curve as a product of the filter sensitivity, CCD, tele...

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Autores: Lorenzo-Gutiérrez, A., Alfaro, Emilio J., Maíz Apellániz, Jesús, Barbá, R. H., Marín-Franch, Antonio, Ederoclite, Alessandro, Cristóbal-Hornillos, David, Varela, Jesús, Vázquez Ramió, H., Cenarro, A. J., Lennon, D. J., García-Lario, P.
Formato: artículo
Estado:Versión publicada
Fecha de publicación:2019
País:España
Recursos:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/193644
Acesso em linha:http://hdl.handle.net/10261/193644
Access Level:acceso abierto
Palavra-chave:Techniques: photometric
Star formation
Galaxies: stars: formation
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spelling The GALANTE photometric systemLorenzo-Gutiérrez, A.Alfaro, Emilio J.Maíz Apellániz, JesúsBarbá, R. H.Marín-Franch, AntonioEderoclite, AlessandroCristóbal-Hornillos, DavidVarela, JesúsVázquez Ramió, H.Cenarro, A. J.Lennon, D. J.García-Lario, P.Techniques: photometricStar formationGalaxies: stars: formationThis paper describes the characterization of the GALANTE photometric system, a seven intermediate-and narrow-band filter system with a wavelength coverage from 3000 Å to 9000 Å. We describe the photometric system presenting the full sensitivity curve as a product of the filter sensitivity, CCD, telescope mirror, and atmospheric transmission curves, as well as some first-and second-order moments of this sensitivity function. The GALANTE photometric system is composed of four filters from the J-PLUS photometric system, a twelve broad-to-narrow filter system, and three exclusive filters, specifically designed to measure the physical parameters of stars such as effective temperature T, log (g), metallicity, colour excess E(4405-5495), and extinction type R. Two libraries, the Next Generation Spectral Library (NGSL) and the one presented in Maíz Apellániz & Weiler (2018), have been used to determine the transformation equations between the Sloan Digital Sky Survey (SDSS) ugriz photometry and the GALANTE photometric system. We will use this transformation to calibrate the zero-points of GALANTE images. To this end, a preliminary photometric calibration of GALANTE has been made based on two different griz libraries (SDSS DR12 and ATLAS All-Sky Stellar Reference Catalog, hereinafter RefCat2). A comparison between both zero-points is performed leading us to the choice of RefCat2 as the base catalogue for this calibration, and applied to a field in the Cyg OB2 association.© 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society.AL-G, EJA, and JMA acknowledge support from the Spanish Government Ministerio de Ciencia, Innovacion y Universidades though grants AYA2013-40 611-P and AYA2016-75 931-C2-1/2-P. A.L.-G and EJA also acknowledge support from the State Agency for Research of the Spanish MCIU through the 'Center of Excellence Severo Ochoa' award for the Instituto de Astrofisica de Andalucia (SEV-2017-0709).Peer ReviewedOxford University PressMinisterio de Economía y Competitividad (España)Ministerio de Ciencia, Innovación y Universidades (España)European CommissionConsejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]2019201920192019info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionhttp://hdl.handle.net/10261/193644reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Inglés#PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE#info:eu-repo/grantAgreement/MINECO/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/AYA2013-40611-Pinfo:eu-repo/grantAgreement/MINECO/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/AYA2016-75931-C2-1-Pinfo:eu-repo/grantAgreement/MINECO/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/SEV-2017-0709info:eu-repo/grantAgreement/MINECO/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/AYA2016-75931-C2-2-Phttp://dx.doi.org/10.1093/mnras/stz842Síinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/1936442026-05-22T06:33:51Z
dc.title.none.fl_str_mv The GALANTE photometric system
title The GALANTE photometric system
spellingShingle The GALANTE photometric system
Lorenzo-Gutiérrez, A.
Techniques: photometric
Star formation
Galaxies: stars: formation
title_short The GALANTE photometric system
title_full The GALANTE photometric system
title_fullStr The GALANTE photometric system
title_full_unstemmed The GALANTE photometric system
title_sort The GALANTE photometric system
dc.creator.none.fl_str_mv Lorenzo-Gutiérrez, A.
Alfaro, Emilio J.
Maíz Apellániz, Jesús
Barbá, R. H.
Marín-Franch, Antonio
Ederoclite, Alessandro
Cristóbal-Hornillos, David
Varela, Jesús
Vázquez Ramió, H.
Cenarro, A. J.
Lennon, D. J.
García-Lario, P.
author Lorenzo-Gutiérrez, A.
author_facet Lorenzo-Gutiérrez, A.
Alfaro, Emilio J.
Maíz Apellániz, Jesús
Barbá, R. H.
Marín-Franch, Antonio
Ederoclite, Alessandro
Cristóbal-Hornillos, David
Varela, Jesús
Vázquez Ramió, H.
Cenarro, A. J.
Lennon, D. J.
García-Lario, P.
author_role author
author2 Alfaro, Emilio J.
Maíz Apellániz, Jesús
Barbá, R. H.
Marín-Franch, Antonio
Ederoclite, Alessandro
Cristóbal-Hornillos, David
Varela, Jesús
Vázquez Ramió, H.
Cenarro, A. J.
Lennon, D. J.
García-Lario, P.
author2_role author
author
author
author
author
author
author
author
author
author
author
dc.contributor.none.fl_str_mv Ministerio de Economía y Competitividad (España)
Ministerio de Ciencia, Innovación y Universidades (España)
European Commission
Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]
dc.subject.none.fl_str_mv Techniques: photometric
Star formation
Galaxies: stars: formation
topic Techniques: photometric
Star formation
Galaxies: stars: formation
description This paper describes the characterization of the GALANTE photometric system, a seven intermediate-and narrow-band filter system with a wavelength coverage from 3000 Å to 9000 Å. We describe the photometric system presenting the full sensitivity curve as a product of the filter sensitivity, CCD, telescope mirror, and atmospheric transmission curves, as well as some first-and second-order moments of this sensitivity function. The GALANTE photometric system is composed of four filters from the J-PLUS photometric system, a twelve broad-to-narrow filter system, and three exclusive filters, specifically designed to measure the physical parameters of stars such as effective temperature T, log (g), metallicity, colour excess E(4405-5495), and extinction type R. Two libraries, the Next Generation Spectral Library (NGSL) and the one presented in Maíz Apellániz & Weiler (2018), have been used to determine the transformation equations between the Sloan Digital Sky Survey (SDSS) ugriz photometry and the GALANTE photometric system. We will use this transformation to calibrate the zero-points of GALANTE images. To this end, a preliminary photometric calibration of GALANTE has been made based on two different griz libraries (SDSS DR12 and ATLAS All-Sky Stellar Reference Catalog, hereinafter RefCat2). A comparison between both zero-points is performed leading us to the choice of RefCat2 as the base catalogue for this calibration, and applied to a field in the Cyg OB2 association.© 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society.
publishDate 2019
dc.date.none.fl_str_mv 2019
2019
2019
2019
dc.type.none.fl_str_mv info:eu-repo/semantics/article
http://purl.org/coar/resource_type/c_6501
Publisher's version
info:eu-repo/semantics/publishedVersion
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/10261/193644
url http://hdl.handle.net/10261/193644
dc.language.none.fl_str_mv Inglés
language_invalid_str_mv Inglés
dc.relation.none.fl_str_mv #PLACEHOLDER_PARENT_METADATA_VALUE#
#PLACEHOLDER_PARENT_METADATA_VALUE#
#PLACEHOLDER_PARENT_METADATA_VALUE#
#PLACEHOLDER_PARENT_METADATA_VALUE#
info:eu-repo/grantAgreement/MINECO/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/AYA2013-40611-P
info:eu-repo/grantAgreement/MINECO/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/AYA2016-75931-C2-1-P
info:eu-repo/grantAgreement/MINECO/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/SEV-2017-0709
info:eu-repo/grantAgreement/MINECO/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/AYA2016-75931-C2-2-P
http://dx.doi.org/10.1093/mnras/stz842
Sí
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.publisher.none.fl_str_mv Oxford University Press
publisher.none.fl_str_mv Oxford University Press
dc.source.none.fl_str_mv reponame:DIGITAL.CSIC. Repositorio Institucional del CSIC
instname:Consejo Superior de Investigaciones Científicas (CSIC)
instname_str Consejo Superior de Investigaciones Científicas (CSIC)
reponame_str DIGITAL.CSIC. Repositorio Institucional del CSIC
collection DIGITAL.CSIC. Repositorio Institucional del CSIC
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