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Ruprecht 147 DANCe I. Members, empirical isochrone, luminosity, and mass distributions
| Indexado |
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| DOI | 10.1051/0004-6361/201834924 | ||||
| Año | 2019 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
Abstract
Conclusions. Our combined Gaia+DANCe data set allows us to obtain an extended list of cluster candidate members, and to derive luminosity, mass, and projected spatial distributions in the oldest open cluster of the solar vicinity.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Olivares, J. | Hombre |
Univ Bordeaux - Francia
Université de Bordeaux - Francia |
| 2 | Bouy, H. | Hombre |
Univ Bordeaux - Francia
Université de Bordeaux - Francia |
| 3 | Sarro, L. M. | - |
UNED - España
Universidad Nacional de Educación a Distancia - España |
| 4 | Miret-Roig, N. | - |
Univ Bordeaux - Francia
Université de Bordeaux - Francia |
| 5 | Berihuete, A. | - |
UNIV CADIZ - España
Universidad de Cádiz - España |
| 6 | Bertin, E. | Hombre |
Inst Astrophys Paris - Francia
UPMC - Francia Institut d 'Astrophysique de Paris - Francia Institut d’Astrophysique de Paris - Francia |
| 7 | Barrado, D. | Hombre |
CSIC - España
Centro de Astrobiología (CSIC-INTA) - España CSIC-INTA - Centro de Astrobiología (CAB) - España |
| 8 | Huelamo, Nuria | Mujer |
CSIC - España
Centro de Astrobiología (CSIC-INTA) - España CSIC-INTA - Centro de Astrobiología (CAB) - España |
| 9 | 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 |
| 10 | Allen, Lori E. | Mujer |
Natl Opt Astron Observ - Estados Unidos
National Optical Astronomy Observatory - Estados Unidos |
| 11 | Beletsky, Y. | Hombre |
Observatorio Las Campanas - Chile
|
| 12 | Serre, S. | - |
Univ Bordeaux - Francia
Université de Bordeaux - Francia |
| 13 | Cuillandre, Jean Charles | Hombre |
Univ Paris Diderot - Francia
Universite Paris 7- Denis Diderot - Francia Institut National des Sciences de l'Univers - Francia INSU - Institut National des Sciences de l'Univers - Francia |
| Fuente |
|---|
| National Science Foundation |
| European Research Council |
| NASA |
| National Aeronautics and Space Administration |
| European Research Council (ERC) under the European Union |
| Space Telescope Science Institute |
| European Space Agency |
| University of California, Los Angeles |
| University of Massachusetts |
| Institute of Technology |
| Association of Canadian Universities for Research in Astronomy |
| Horizon 2020 Framework Programme |
| Association of Universities for Research in Astronomy, Inc. |
| Jet Propulsion Laboratory/California Institute of Technology |
| European Union’s Horizon 2020 research and innovation programme |
| French State in the framework of the "Investments for the future" Program, IdEx Bordeaux |
| P.I. |
| ANR-10-IDEX-03-02 |
| IdEx Bordeaux |
| Agradecimiento |
|---|
| We acknowledge Jason Lee Curtis for his kind comments, which considerably improved the quality of this work. 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 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 catalog 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. Some/all of the data presented in this paper were obtained from the Mikulski Archive for Space Telescopes (MAST). STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. |
| Acknowledgements. We acknowledge Jason Lee Curtis for his kind comments, which considerably improved the quality of this work. 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 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 catalog 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. Some/all of the data presented in this paper were obtained from the Mikulski Archive for Space Telescopes (MAST). STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. |
