GALACTICNUCLEUS: A high-angular-resolution JHK simaging survey of the Galactic centre: IV. Extinction maps and de-reddened photometry
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. Open Access funding p...
| Autores: | , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2022 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/259964 |
| Acceso en línea: | http://hdl.handle.net/10261/259964 |
| Access Level: | acceso abierto |
| Palabra clave: | Galaxy: center Galaxy: bulge Galaxy: structure Stars: horizontal-branch Dust Extinction |
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GALACTICNUCLEUS: A high-angular-resolution JHK simaging survey of the Galactic centre: IV. Extinction maps and de-reddened photometry |
| title |
GALACTICNUCLEUS: A high-angular-resolution JHK simaging survey of the Galactic centre: IV. Extinction maps and de-reddened photometry |
| spellingShingle |
GALACTICNUCLEUS: A high-angular-resolution JHK simaging survey of the Galactic centre: IV. Extinction maps and de-reddened photometry Nogueras-Lara, Francisco Galaxy: center Galaxy: bulge Galaxy: structure Stars: horizontal-branch Dust Extinction |
| title_short |
GALACTICNUCLEUS: A high-angular-resolution JHK simaging survey of the Galactic centre: IV. Extinction maps and de-reddened photometry |
| title_full |
GALACTICNUCLEUS: A high-angular-resolution JHK simaging survey of the Galactic centre: IV. Extinction maps and de-reddened photometry |
| title_fullStr |
GALACTICNUCLEUS: A high-angular-resolution JHK simaging survey of the Galactic centre: IV. Extinction maps and de-reddened photometry |
| title_full_unstemmed |
GALACTICNUCLEUS: A high-angular-resolution JHK simaging survey of the Galactic centre: IV. Extinction maps and de-reddened photometry |
| title_sort |
GALACTICNUCLEUS: A high-angular-resolution JHK simaging survey of the Galactic centre: IV. Extinction maps and de-reddened photometry |
| dc.creator.none.fl_str_mv |
Nogueras-Lara, Francisco Schödel, Rainer Neumayer, N. |
| author |
Nogueras-Lara, Francisco |
| author_facet |
Nogueras-Lara, Francisco Schödel, Rainer Neumayer, N. |
| author_role |
author |
| author2 |
Schödel, Rainer Neumayer, N. |
| author2_role |
author author |
| dc.contributor.none.fl_str_mv |
Federal Ministry of Education and Research (Germany) German Research Foundation European Commission Ministerio de Economía y Competitividad (España) Ministerio de Ciencia, Innovación y Universidades (España) Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72] |
| dc.subject.none.fl_str_mv |
Galaxy: center Galaxy: bulge Galaxy: structure Stars: horizontal-branch Dust Extinction |
| topic |
Galaxy: center Galaxy: bulge Galaxy: structure Stars: horizontal-branch Dust Extinction |
| description |
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. Open Access funding provided by Max Planck Society. |
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2022 |
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2022 2022 2022 |
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info:eu-repo/semantics/article http://purl.org/coar/resource_type/c_6501 Publisher's version info:eu-repo/semantics/publishedVersion |
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article |
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http://hdl.handle.net/10261/259964 |
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http://hdl.handle.net/10261/259964 |
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Inglés |
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Inglés |
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EDP Sciences |
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EDP Sciences |
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GALACTICNUCLEUS: A high-angular-resolution JHK simaging survey of the Galactic centre: IV. Extinction maps and de-reddened photometryNogueras-Lara, FranciscoSchödel, RainerNeumayer, N.Galaxy: centerGalaxy: bulgeGalaxy: structureStars: horizontal-branchDustExtinctionOpen Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. Open Access funding provided by Max Planck Society.Context. The extreme extinction (AV ~ 30 mag) and its variation on arc-second scales towards the Galactic centre hamper the study of its stars. Analysis of them is restricted to the near infrared (NIR) regime, where the extinction curve can be approximated by a broken power law for the JHKs bands. Therefore, it is fundamental to correct for extinction at these wavelengths in order to analyse the structure and stellar population of the central regions of our Galaxy. Aims. We aim to, (1) discuss different strategies to de-redden the photometry and check the usefulness of extinction maps to deal with variable stars; (2) build extinction maps for the NIR bands JHKs and make them publicly available; (3) create a de-reddened catalogue of the GALACTICNUCLEUS (GNS) survey, identifying foreground stars; and (4) perform a preliminary analysis of the de-reddened Ks luminosity functions (KLFs). Methods. We used photometry from the GNS survey to create extinction maps for the whole catalogue. We took red clump (RC) and red giant stars of similar brightnesses as a reference to build the maps and we de-reddened the GNS photometry. We also discussed the limitations of the process and analysed non-linear effects of the de-reddening. Results. We obtained high resolution (~3″) extinction maps with low statistical and systematics uncertainties (5%) and computed average extinctions for each of the regions covered by the GNS. We checked that our maps effectively correct the differential extinction reducing the spread of the RC features by a factor of ~2. We assessed the validity of the broken power law approach computing two equivalent extinction maps AH using either JH and HKs photometry for the same reference stars and obtained compatible average extinctions within the uncertainties. Finally, we analysed de-reddened KLFs for different lines of sight and found that the regions belonging to the NSD contain a homogeneous stellar population that is significantly different from that in the innermost bulge regions. © F. Nogueras-Lara et al. 2021.This work is based on observations made with ESO Telescopes at the La Silla Paranal Observatory under program ID 195.B-0283. We thank the staff of ESO for their great efforts and helpfulness. F.N.-L. acknowledges the sponsorship provided by the Federal Ministry for Education and Research of Germany through the Alexander von Humboldt Foundation. F.N.-L. and N.N. gratefully acknowledge support by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) - Project-ID 138713538 - SFB 881 ("The Milky Way System", subproject B8). R.S. acknowledges financial 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). R.S. acknowledges financial support from national project PGC2018-095049-B-C21 (MCIU/AEI/FEDER, UE).Peer reviewedEDP SciencesFederal Ministry of Education and Research (Germany)German Research FoundationEuropean CommissionMinisterio de Economía y Competitividad (España)Ministerio de Ciencia, Innovación y Universidades (España)Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]202220222022info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionhttp://hdl.handle.net/10261/259964reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Inglés#PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE#info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PGC2018-095049-B-C21info:eu-repo/grantAgreement/MICINN//SEV-2017-0709http://dx.doi.org/10.1051/0004-6361/202140996Síinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/2599642026-05-22T06:33:51Z |
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