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Consultas o comentarios: productividad@anid.cl
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IC 4665 DANCe I. Members, empirical isochrones, magnitude distributions, present-day system mass function, and spatial distribution
| Indexado |
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| DOI | 10.1051/0004-6361/201935518 | ||||
| Año | 2019 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
Abstract
Conclusions. Our membership analysis represents a significant increase in the quantity and quality (low contamination) with respect to previous studies. It o ffers an excellent opportunity to revisit other fundamental parameters such as age.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Miret-Roig, N. | - |
Univ Bordeaux - Francia
Université de Bordeaux - Francia |
| 2 | Bouy, H. | Hombre |
Univ Bordeaux - Francia
Université de Bordeaux - Francia |
| 3 | Olivares, J. | Hombre |
Univ Bordeaux - Francia
Université de Bordeaux - Francia |
| 4 | Sarro, L. M. | - |
UNED - España
Universidad Nacional de Educación a Distancia - España |
| 5 | Tamura, Motohide | - |
Univ Tokyo - Japón
Natl Astron Observ Japan - Japón Astrobiol Ctr - Japón University of Tokyo - Japón National Institutes of Natural Sciences - National Astronomical Observatory of Japan - Japón Astrobiology Center - Japón The University of Tokyo - Japón National Institutes of Natural Sciences - AstroBiology Center - Japón |
| 6 | Allen, Lori E. | Mujer |
Natl Opt Astron Observ - Estados Unidos
National Optical Astronomy Observatory - Estados Unidos |
| 7 | Bertin, E. | Hombre |
CNRS UMR 7095 - Francia
UPMC - Francia Institut d 'Astrophysique de Paris - Francia Institut d’Astrophysique de Paris - Francia |
| 8 | Serre, S. | - |
Univ Bordeaux - Francia
Université de Bordeaux - Francia |
| 9 | Berihuete, A. | - |
UNIV CADIZ - España
Universidad de Cádiz - España |
| 10 | Beletsky, Y. | Hombre |
Carnegie Inst Sci - Chile
|
| 11 | Barrado, D. | Hombre |
Ctr Astrobiol CSIC INTA - España
Centro de Astrobiología (CSIC-INTA) - España CSIC-INTA - Centro de Astrobiología (CAB) - España |
| 12 | Huelamo, Nuria | Mujer |
Ctr Astrobiol CSIC INTA - España
Centro de Astrobiología (CSIC-INTA) - España CSIC-INTA - Centro de Astrobiología (CAB) - España |
| 13 | Cuillandre, Jean Charles | Hombre |
Univ Paris Diderot - Francia
Universite Paris 7- Denis Diderot - Francia Institut National des Sciences de l'Univers - Francia Commissariat a l'Energie Atomique et aux Energies Alternatives - Francia |
| 14 | Moraux, E. | Mujer |
Univ Grenoble Alpes - Francia
Universite Grenoble Alpes - Francia |
| 15 | Bouvier, J. | Hombre |
Univ Grenoble Alpes - Francia
Universite Grenoble Alpes - Francia |
| Fuente |
|---|
| National Science Foundation |
| European Research Council |
| National Aeronautics and Space Administration |
| European Research Council (ERC) under the European Union |
| European Space Agency |
| Agencia Estatal de Investigación |
| University of California, Los Angeles |
| University of Massachusetts |
| Institute of Technology |
| Association of Canadian Universities for Research in Astronomy |
| "Investments for the future" Program, IdEx Bordeaux |
| MEXT/JSPS KAKENHI |
| Spanish State Research Agency (AEI) Unidad de Excelencia "Maria de Maeztu" Centro de Astrobiologia (INTA-CSIC) |
| ESO programmes |
| Australian Education International, Australian Government |
| Horizon 2020 Framework Programme |
| Jet Propulsion Laboratory/California Institute of Technology |
| European Union’s Horizon 2020 research and innovation programme |
| P.I. |
| MEXT/JSPS |
| MEXT/JSPS KAK-ENHI |
| ANR-10-IDEX-03-02 |
| IdEx Bordeaux |
| Agradecimiento |
|---|
| We thank the referee for the thorough review and highly appreciate the comments and suggestions that significantly contributed to improving the quality of the publication. We are grateful to Ingo Thies for sharing with us his models of the Initial Mass Function, to France Allard and Isabelle Barra ffe for providing us with the latest version of the BTSettl models, and to Paul Price for his help with the LSST/HSC pipeline. This research has received funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme (grant agreement No 682903, P.I. H. Bouy), and from the French State in the framework of the "Investments for the future" Program, IdEx Bordeaux, reference ANR-10-IDEX-03-02. This project has been funded by the Spanish State Research Agency (AEI) Project No. ESP2017-87676-C5-1-R and No. MDM-2017-0737 Unidad de Excelencia "Maria de Maeztu" Centro de Astrobiologia (INTA-CSIC). M.T. is supported by MEXT/JSPS KAKENHI grant Nos. 18H05442, 15H02063, and 22000005. Based on observations collected at the European Southern Observatory under ESO programmes 60.A-9120(A), 60.A-9121(A), 60.A-9122(A), 68.C-0311(A), 69.A-9014(A), 69.C-0034(A), 69.C-0260(A), 69.C-0398(B), 69.C-0426(C), 69.D-0582(A), 60.A-9038(A). This research draws upon data distributed by the NOAO Science Archive. NOAO is operated by the Association of Universities for Research in Astronomy (AURA) under cooperative agreement with the National Science Foundation. This publication makes use of data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation. This work has made use of data from the European Space Agency (ESA) mission Gaia (http://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, http://www.cosmos.esa.int/web/gaia/dpac/consortium).Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. This research has made use of the VizieR and Aladin images and catalogue access tools and of the SIMBAD database, operated at the CDS, Strasbourg, France. This publication makes use of data products from the Wide-field Infrared Survey Explorer, which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory/California Institute of Technology, funded by the National Aeronautics and Space Administration. This research has made use of GNU Parallel (Tange 2011), Astropy (Astropy Collaboration 2013), Topcat (Taylor 2005), STILTS (Taylor 2006). |
| Acknowledgements. We thank the referee for the thorough review and highly appreciate the comments and suggestions that significantly contributed to improving the quality of the publication. We are grateful to Ingo Thies for sharing with us his models of the Initial Mass Function, to France Allard and Isabelle Barraffe for providing us with the latest version of the BT-Settl models, and to Paul Price for his help with the LSST/HSC pipeline. This research has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement No 682903, P.I. H. Bouy), and from the French State in the framework of the “Investments for the future” Program, IdEx Bordeaux, reference ANR-10-IDEX-03-02 . This project has been funded by the Spanish State Research Agency (AEI) Project No. ESP2017-87676-C5-1-R and No. MDM-2017-0737 Unidad de Excelencia “María de Maeztu” Centro de Astrobiología (INTA-CSIC). M.T. is supported by MEXT/JSPS KAK-ENHI grant Nos. 18H05442, 15H02063, and 22000005. Based on observations collected at the European Southern Observatory under ESO programmes 60.A-9120(A), 60.A-9121(A), 60.A-9122(A), 68.C-0311(A), 69.A-9014(A), 69.C-0034(A), 69.C-0260(A), 69.C-0398(B), 69.C-0426(C), 69.D-0582(A), 60.A-9038(A). This research draws upon data distributed by the NOAO Science Archive. NOAO is operated by the Association of Universities for Research in Astronomy (AURA) under cooperative agreement with the National Science Foundation. This publication makes use of data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation. This work has made use of data from the European Space Agency (ESA) mission Gaia (http://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, http://www.cosmos.esa.int/web/gaia/dpac/consortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. This research has made use of the VizieR and Aladin images and catalogue access tools and of the SIMBAD database, operated at the CDS, Strasbourg, France. This publication makes use of data products from the Wide-field Infrared Survey Explorer, which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory/California Institute of Technology, funded by the National Aeronautics and Space Administration. This research has made use of GNU Parallel (Tange 2011), Astropy (Astropy Collaboration 2013), Topcat (Taylor 2005), STILTS (Taylor 2006). |
