The Calar Alto Legacy Integral Field Area survey: extended and remastered data release

This paper describes the extended data release (eDR) of the Calar Alto Legacy Integral Field Area (CALIFA) survey. It comprises science-grade quality data for 895 galaxies obtained with the Potsdam Multi Aperture Spectograph/PPak instrument at the 3.5-m telescope at the Calar Alto Observatory along...

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Detalhes bibliográficos
Autores: Sánchez, Sebastián F., Galbany, Lluís, Walcher, C. J., García-Benito, Rubén, Barrera-Ballesteros, Jorge K.
Formato: artículo
Estado:Versión publicada
Fecha de publicación:2023
País:España
Recursos:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/348935
Acesso em linha:http://hdl.handle.net/10261/348935
Access Level:acceso abierto
Palavra-chave:Techniques: spectroscopic
Galaxies: evolution
Galaxies: ISM
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dc.title.none.fl_str_mv The Calar Alto Legacy Integral Field Area survey: extended and remastered data release
title The Calar Alto Legacy Integral Field Area survey: extended and remastered data release
spellingShingle The Calar Alto Legacy Integral Field Area survey: extended and remastered data release
Sánchez, Sebastián F.
Techniques: spectroscopic
Galaxies: evolution
Galaxies: ISM
title_short The Calar Alto Legacy Integral Field Area survey: extended and remastered data release
title_full The Calar Alto Legacy Integral Field Area survey: extended and remastered data release
title_fullStr The Calar Alto Legacy Integral Field Area survey: extended and remastered data release
title_full_unstemmed The Calar Alto Legacy Integral Field Area survey: extended and remastered data release
title_sort The Calar Alto Legacy Integral Field Area survey: extended and remastered data release
dc.creator.none.fl_str_mv Sánchez, Sebastián F.
Galbany, Lluís
Walcher, C. J.
García-Benito, Rubén
Barrera-Ballesteros, Jorge K.
author Sánchez, Sebastián F.
author_facet Sánchez, Sebastián F.
Galbany, Lluís
Walcher, C. J.
García-Benito, Rubén
Barrera-Ballesteros, Jorge K.
author_role author
author2 Galbany, Lluís
Walcher, C. J.
García-Benito, Rubén
Barrera-Ballesteros, Jorge K.
author2_role author
author
author
author
dc.contributor.none.fl_str_mv Ministerio de Ciencia, Innovación y Universidades (España)
Consejo Nacional de Ciencia y Tecnología (México)
European Commission
Agencia Estatal de Investigación (España)
Ministerio de Ciencia e Innovación (España)
Consejo Superior de Investigaciones Científicas (España)
Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]
dc.subject.none.fl_str_mv Techniques: spectroscopic
Galaxies: evolution
Galaxies: ISM
topic Techniques: spectroscopic
Galaxies: evolution
Galaxies: ISM
description This paper describes the extended data release (eDR) of the Calar Alto Legacy Integral Field Area (CALIFA) survey. It comprises science-grade quality data for 895 galaxies obtained with the Potsdam Multi Aperture Spectograph/PPak instrument at the 3.5-m telescope at the Calar Alto Observatory along the last 12 yr, using the V500 setup [3700–7500 Å, 6 Å/full-width at half-maximum (FWHM)] and the CALIFA observing strategy. It includes galaxies of any morphological type, star formation stage, a wide range of stellar masses (∼107–1012 M⊙), at an average redshift of ∼0.015 (90 per cent within 0.005 < z < 0.05). Primarily selected based on the projected size and apparent magnitude, we demonstrate that it can be volume corrected resulting in a statistically limited but representative sample of the population of galaxies in the nearby Universe. All the data were homogeneous re-reduced, introducing a set of modifications to the previous reduction. The most relevant is the development and implementation of a new cube-reconstruction algorithm that provides with an (almost) seeing-limited spatial resolution (FWHMPSF ∼ 1.0 arcsec). To illustrate the usability and quality of the data, we extracted two aperture spectra for each galaxy (central 1.5 arcsec and fully integrated), and analyse them using PYFIT3D. We obtain a set of observational and physical properties of both the stellar populations and the ionized gas, that have been compared for the two apertures, exploring their distributions as a function of the stellar masses and morphologies of the galaxies, comparing with recent results in the literature.
publishDate 2023
dc.date.none.fl_str_mv 2023
2024
2024
dc.type.none.fl_str_mv info:eu-repo/semantics/article
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The underlying dataset has been published as supplementary material of the article in the publisher platform at DOI 10.1093/mnras/stad3119
https://doi.org/10.1093/mnras/stad3119
Sí
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dc.publisher.none.fl_str_mv Oxford University Press
publisher.none.fl_str_mv Oxford University Press
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spelling The Calar Alto Legacy Integral Field Area survey: extended and remastered data releaseSánchez, Sebastián F.Galbany, LluísWalcher, C. J.García-Benito, RubénBarrera-Ballesteros, Jorge K.Techniques: spectroscopicGalaxies: evolutionGalaxies: ISMThis paper describes the extended data release (eDR) of the Calar Alto Legacy Integral Field Area (CALIFA) survey. It comprises science-grade quality data for 895 galaxies obtained with the Potsdam Multi Aperture Spectograph/PPak instrument at the 3.5-m telescope at the Calar Alto Observatory along the last 12 yr, using the V500 setup [3700–7500 Å, 6 Å/full-width at half-maximum (FWHM)] and the CALIFA observing strategy. It includes galaxies of any morphological type, star formation stage, a wide range of stellar masses (∼107–1012 M⊙), at an average redshift of ∼0.015 (90 per cent within 0.005 < z < 0.05). Primarily selected based on the projected size and apparent magnitude, we demonstrate that it can be volume corrected resulting in a statistically limited but representative sample of the population of galaxies in the nearby Universe. All the data were homogeneous re-reduced, introducing a set of modifications to the previous reduction. The most relevant is the development and implementation of a new cube-reconstruction algorithm that provides with an (almost) seeing-limited spatial resolution (FWHMPSF ∼ 1.0 arcsec). To illustrate the usability and quality of the data, we extracted two aperture spectra for each galaxy (central 1.5 arcsec and fully integrated), and analyse them using PYFIT3D. We obtain a set of observational and physical properties of both the stellar populations and the ionized gas, that have been compared for the two apertures, exploring their distributions as a function of the stellar masses and morphologies of the galaxies, comparing with recent results in the literature.SFS thanks the PAPIIT-DGAPA AG100622 project. JKBB and SFS acknowledge support from the CONACYT grant CF19-39578. RGB acknowledges financial support from the grants CEX2021-001131-S funded by MCIN/AEI/10.13039/501100011033, SEV-2017-0709, and to PID2019-109067-GB100. LG acknowledges financial support from the Spanish Ministerio de Ciencia e Innovación (MCIN), the Agencia Estatal de Investigación (AEI) 10.13039/501100011033, and the European Social Fund (ESF) ‘Investing in your future’ under the 2019 Ramón y Cajal program RYC2019-027683-I and the PID2020-115253GA-I00 HOSTFLOWS project, from Centro Superior de Investigaciones Científicas (CSIC) under the PIE project 20215AT016, and the program Unidad de Excelencia María de Maeztu CEX2020-001058-M.With funding from the Spanish government through the "Severo Ochoa Centre of Excellence" accreditation (CEX2021-001131-S).With funding from the Spanish government through the "Severo Ochoa Centre of Excellence" accreditation (CEX2020-001058-M).Peer reviewedOxford University PressMinisterio de Ciencia, Innovación y Universidades (España)Consejo Nacional de Ciencia y Tecnología (México)European CommissionAgencia Estatal de Investigación (España)Ministerio de Ciencia e Innovación (España)Consejo Superior de Investigaciones Científicas (España)Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]202420242023info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionapplication/pdfhttp://hdl.handle.net/10261/348935reponame: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##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE#info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/CEX2021-001131-Sinfo:eu-repo/grantAgreement/AEI//SEV-2017-0709info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PID2019-109067GB-I00info:eu-repo/grantAgreement/AEI//RYC2019-027683-Iinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/CEX2020-001058-Minfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PID2020-115253GA-I00The underlying dataset has been published as supplementary material of the article in the publisher platform at DOI 10.1093/mnras/stad3119https://doi.org/10.1093/mnras/stad3119Síinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/3489352026-05-22T06:33:51Z
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