Dataciencia

Colección SciELO Chile

Stellar parameters for stars of the CoRoT exoplanet field

Indexado

WoS	WOS:000361803900068
Scopus	SCOPUS_ID:84940991056

DOI

10.1051/0004-6361/201424155

Año

2015

Tipo

artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras

Abstract

Conclusions. Our spectroscopic catalog, by providing much-needed spectroscopic information for a large sample of CoRoT targets, will be of key importance for the successful accomplishment of several different programs related to the CoRoT mission, thus it will help further boost the scientific return associated with this space mission.

Revista

Revista	ISSN
Astronomy & Astrophysics	0004-6361

Métricas Externas

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Disciplinas de Investigación

WOS
Astronomy & Astrophysics

Scopus
Sin Disciplinas

SciELO
Sin Disciplinas

Muestra la distribución de disciplinas para esta publicación.

Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional

Muestra la distribución de colaboración, tanto nacional como extranjera, generada en esta publicación.

Autores - Afiliación

Ord.	Autor	Género	Institución - País
1	CORTES-ORELLANA, CADDY CORAL	Hombre	Universidad Metropolitana de Ciencias de la Educación - Chile Univ Fed Rio Grande do Norte - Brasil Instituto Milenio de Astrofísica - Chile Universidade Federal do Rio Grande do Norte - Brasil Santiago - Chile
2	Maciel, S. C.	-	Univ Fed Rio Grande do Norte - Brasil Universidade Federal do Rio Grande do Norte - Brasil
3	Vieira, S.	-	Univ Fed Rio Grande do Norte - Brasil Univ Fed Roraima - Brasil Universidade Federal do Rio Grande do Norte - Brasil Universidade Federal de Roraima - Brasil
4	Ferreira Lopes, C. E.	Hombre	Univ Fed Rio Grande do Norte - Brasil UNIV EDINBURGH - Reino Unido Universidade Federal do Rio Grande do Norte - Brasil University of Edinburgh, Institute for Astronomy - Reino Unido
5	Leao, I.	-	Univ Fed Rio Grande do Norte - Brasil Universidade Federal do Rio Grande do Norte - Brasil
6	Pereira de Oliveira, G.	-	Univ Fed Rio Grande do Norte - Brasil Universidade Federal do Rio Grande do Norte - Brasil
7	Carrasco-Gonzalez, Carlos	Hombre	Univ Fed Rio Grande do Norte - Brasil Universidade Federal do Rio Grande do Norte - Brasil
8	Martins, B. L. Canto	Hombre	Univ Fed Rio Grande do Norte - Brasil Universidade Federal do Rio Grande do Norte - Brasil
9	Catelan, Marcio	Hombre	Instituto Milenio de Astrofísica - Chile Pontificia Universidad Católica de Chile - Chile Centro de Excelencia en Astrofísica y Tecnologías Afines - Chile Santiago - Chile
10	de Medeiros, Jose R.	Hombre	Univ Fed Rio Grande do Norte - Brasil Universidade Federal do Rio Grande do Norte - Brasil

Muestra la afiliación y género (detectado) para los co-autores de la publicación.

Financiamiento

Fuente
CNPq
Conselho Nacional de Desenvolvimento Científico e Tecnológico
Fondo Nacional de Desarrollo Científico y Tecnológico
Coordenação de Aperfeiçoamento de Pessoal de Nível Superior
Proyecto Basal
Deutsche Forschungsgemeinschaft
National Aeronautics and Space Administration
Fondo Nacional de Desarrollo CientÃfico y TecnolÃ³gico
Proyecto FONDECYT
CoordenaÃ§Ã£o de AperfeiÃ§oamento de Pessoal de NÃvel Superior
Conselho Nacional de Desenvolvimento CientÃfico e TecnolÃ³gico
CAPES agency
Chilean Ministry for the Economy, Development, and Tourism's Programa Iniciativa Cientifica Milenio
FundaÃ§Ã£o de Apoio Ã Pesquisa do Rio Grande do Norte
Ministry for the Economy, Development
FAPERN
German Deutsche Forschungsgemeinschaft, DFG
German Deutsche Forschungsgemeinschaft
INCT INEspaco
Fundação de Apoio à Pesquisa do Rio Grande do Norte

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos

Agradecimiento
Research activities of the Stellar Board of the Federal University of Rio Grande do Norte are supported by continuous grants of CNPq and FAPERN Brazilian agencies. We also acknowledges financial support of the INCT INEspaco. I.C.L. and C.E.F.L. acknowledges postdoctoral fellowship of the CNPq; C.C., S.C.M., C.E.F.L., S.V. and G.P.O. acknowledge graduate fellowships of the CAPES agency. This work was partially supported by the German Deutsche Forschungsgemeinschaft, DFG project number Ts 17/201. Support for C.C. and M.C. is provided by the Chilean Ministry for the Economy, Development, and Tourism's Programa Iniciativa Cientifica Milenio through grant IC 120009, awarded to the Millennium Institute of Astrophysics (MAS); by Proyecto Basal PFB- 06/2007; and by Proyecto FONDECYT Regular #1141141. This research has made use of the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.
Research activities of the Stellar Board of the Federal University of Rio Grande do Norte are supported by continuous grants of CNPq and FAPERN Brazilian agencies. We also acknowledges financial support of the INCT INEspaço. I.C.L. and C.E.F.L. acknowledges postdoctoral fellowship of the CNPq; C.C., S.C.M., C.E.F.L., S.V. and G.P.O. acknowledge graduate fellowships of the CAPES agency. This work was partially supported by the German Deutsche Forschungsgemeinschaft, DFG project number Ts 17/201. Support for C.C. and M.C. is provided by the Chilean Ministry for the Economy, Development, and Tourism’s Programa Iniciativa Científica Milenio through grant IC 120009, awarded to the Millennium Institute of Astrophysics (MAS); by Proyecto Basal PFB- 06/2007; and by Proyecto FONDECYT Regular #1141141. This research has made use of the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.

Agradecimiento

Research activities of the Stellar Board of the Federal University of Rio Grande do Norte are supported by continuous grants of CNPq and FAPERN Brazilian agencies. We also acknowledges financial support of the INCT INEspaco. I.C.L. and C.E.F.L. acknowledges postdoctoral fellowship of the CNPq; C.C., S.C.M., C.E.F.L., S.V. and G.P.O. acknowledge graduate fellowships of the CAPES agency. This work was partially supported by the German Deutsche Forschungsgemeinschaft, DFG project number Ts 17/201. Support for C.C. and M.C. is provided by the Chilean Ministry for the Economy, Development, and Tourism's Programa Iniciativa Cientifica Milenio through grant IC 120009, awarded to the Millennium Institute of Astrophysics (MAS); by Proyecto Basal PFB- 06/2007; and by Proyecto FONDECYT Regular #1141141. This research has made use of the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.

Research activities of the Stellar Board of the Federal University of Rio Grande do Norte are supported by continuous grants of CNPq and FAPERN Brazilian agencies. We also acknowledges financial support of the INCT INEspaço. I.C.L. and C.E.F.L. acknowledges postdoctoral fellowship of the CNPq; C.C., S.C.M., C.E.F.L., S.V. and G.P.O. acknowledge graduate fellowships of the CAPES agency. This work was partially supported by the German Deutsche Forschungsgemeinschaft, DFG project number Ts 17/201. Support for C.C. and M.C. is provided by the Chilean Ministry for the Economy, Development, and Tourism’s Programa Iniciativa Científica Milenio through grant IC 120009, awarded to the Millennium Institute of Astrophysics (MAS); by Proyecto Basal PFB- 06/2007; and by Proyecto FONDECYT Regular #1141141. This research has made use of the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.