The ALHAMBRA Photometric System

This paper presents the characterization of the optical range of the ALHAMBRA photometric system, a 20 contiguous, equal-width, medium-band CCD system with wavelength coverage from 3500A to 9700A. The photometric description of the system is done by presenting the full response curve as a product of...

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Detalles Bibliográficos
Autores: Aparicio Villegas, T., Infante, L.
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2010
País:Chile
Idioma:inglés
OAI Identifier:oai:repositorio.anid.cl:10533/237095
Acceso en línea:https://hdl.handle.net/10533/237095
Access Level:acceso abierto
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spelling Infante, L.Aparicio Villegas, T.201010.1088/0004-6256/139/3/1242https://hdl.handle.net/10533/237095http://purl.org/coar/access_right/c_abf2The ALHAMBRA Photometric SystemAparicio Villegas, T.Infante, L.2019-12-18T18:14:45Z2022-07-07T22:03:30Z2019-12-18T18:14:45Z2022-07-07T22:03:30Z2010This paper presents the characterization of the optical range of the ALHAMBRA photometric system, a 20 contiguous, equal-width, medium-band CCD system with wavelength coverage from 3500A to 9700A. The photometric description of the system is done by presenting the full response curve as a product of the filters, CCD and atmospheric transmission curves, and using some first and second order moments of this response function. We also introduce the set of standard stars that defines the system, formed by 31 classic spectrophotometric standard stars which have been used in the calibration of other known photometric systems, and 288 stars, flux calibrated homogeneously, from the Next Generation Spectral Library (NGSL). Based on the NGSL, we determine the transformation equations between Sloan Digital Sky Survey (SDSS) ugriz photometry and the ALHAMBRA photometric system, in order to establish some relations between both systems. Finally we develop and discuss a strategy to calculate the photometric zero points of the different pointings in the ALHAMBRA project. Comment: Astronomical Journal on the 14th of January 2010.FONDAPFONDAP1501000315010003virtual::14606-1WOS:000274429600034https://hdl.handle.net/10533/237095enginstname: Conicytreponame: Repositorio Digital RI2.010.1088/0004-6256/139/3/1242info:eu-repo/grantAgreement/Fondap/15010003https://www.researchgate.net/publication/45896251_The_ALHAMBRA_photometric_systemAtribución-NoComercial-SinDerivadas 3.0 Chilehttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/info:eu-repo/semantics/openAccessThe ALHAMBRA Photometric SystemAstronomical JournalArticuloinfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttps://hdl.handle.net/10533/237095http://purl.org/coar/resource_type/c_2df8fbb1045fc0e1-ef55-4532-8afe-69fe789d964dvirtual::14606-1045fc0e1-ef55-4532-8afe-69fe789d964dvirtual::14606-110533/237095oai:repositorio.anid.cl:10533/2370952023-07-24 18:53:55.708https://repositorio.anid.clRepositorio ANIDaletelier@anid.cl
dc.title.none.fl_str_mv The ALHAMBRA Photometric System
dc.title.journal.none.fl_str_mv Astronomical Journal
title The ALHAMBRA Photometric System
spellingShingle The ALHAMBRA Photometric System
Aparicio Villegas, T.
title_short The ALHAMBRA Photometric System
title_full The ALHAMBRA Photometric System
title_fullStr The ALHAMBRA Photometric System
title_full_unstemmed The ALHAMBRA Photometric System
title_sort The ALHAMBRA Photometric System
dc.creator.none.fl_str_mv Aparicio Villegas, T.
Infante, L.
author Aparicio Villegas, T.
author_facet Aparicio Villegas, T.
Infante, L.
author_role author
author2 Infante, L.
author2_role author
description This paper presents the characterization of the optical range of the ALHAMBRA photometric system, a 20 contiguous, equal-width, medium-band CCD system with wavelength coverage from 3500A to 9700A. The photometric description of the system is done by presenting the full response curve as a product of the filters, CCD and atmospheric transmission curves, and using some first and second order moments of this response function. We also introduce the set of standard stars that defines the system, formed by 31 classic spectrophotometric standard stars which have been used in the calibration of other known photometric systems, and 288 stars, flux calibrated homogeneously, from the Next Generation Spectral Library (NGSL). Based on the NGSL, we determine the transformation equations between Sloan Digital Sky Survey (SDSS) ugriz photometry and the ALHAMBRA photometric system, in order to establish some relations between both systems. Finally we develop and discuss a strategy to calculate the photometric zero points of the different pointings in the ALHAMBRA project. Comment: Astronomical Journal on the 14th of January 2010.
publishDate 2010
dc.date.issued.none.fl_str_mv 2010
dc.date.accessioned.none.fl_str_mv 2019-12-18T18:14:45Z
2022-07-07T22:03:30Z
dc.date.available.none.fl_str_mv 2019-12-18T18:14:45Z
2022-07-07T22:03:30Z
dc.type.none.fl_str_mv Articulo
dc.type.driver.none.fl_str_mv info:eu-repo/semantics/article
dc.type.openaire.none.fl_str_mv info:eu-repo/semantics/publishedVersion
format article
status_str publishedVersion
dc.identifier.folio.none.fl_str_mv 15010003
15010003
dc.identifier.idwos.none.fl_str_mv WOS:000274429600034
dc.identifier.uri.none.fl_str_mv https://hdl.handle.net/10533/237095
identifier_str_mv 15010003
WOS:000274429600034
url https://hdl.handle.net/10533/237095
dc.language.iso.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv instname: Conicyt
reponame: Repositorio Digital RI2.0
dc.relation.doi.none.fl_str_mv 10.1088/0004-6256/139/3/1242
dc.relation.projectid.none.fl_str_mv info:eu-repo/grantAgreement/Fondap/15010003
dc.relation.uri.none.fl_str_mv https://www.researchgate.net/publication/45896251_The_ALHAMBRA_photometric_system
dc.rights.none.fl_str_mv Atribución-NoComercial-SinDerivadas 3.0 Chile
http://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.rights.driver.none.fl_str_mv info:eu-repo/semantics/openAccess
rights_invalid_str_mv Atribución-NoComercial-SinDerivadas 3.0 Chile
http://creativecommons.org/licenses/by-nc-nd/3.0/cl/
eu_rights_str_mv openAccess
repository.name.fl_str_mv Repositorio ANID
repository.mail.fl_str_mv aletelier@anid.cl
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