Dataciencia

Colección SciELO Chile

Near-infrared photometry of Galactic planetary nebulae with the VVV Survey

Indexado

WoS	WOS:000317912000074
Scopus	SCOPUS_ID:84875750414

DOI

10.1051/0004-6361/201220492

Año

2013

Tipo

artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras

Abstract

Conclusions. The VVV survey represents a unique dataset for studying crowded and obscured regions in the Galactic plane. The diagnostic diagrams presented here allow one to study the properties of known PNe and to uncover objects not previously classified.

Revista

Revista	ISSN
Astronomy & Astrophysics	1432-0746

Métricas Externas

PlumX	Altmetric	Dimensions

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Disciplinas de Investigación

WOS
Astronomy & Astrophysics

Scopus
Sin Disciplinas

SciELO
Sin Disciplinas

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

Colaboración Institucional

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Autores - Afiliación

Ord.	Autor	Género	Institución - País
1	Weidmann, W.	Hombre	UNIV NACL CORDOBA - Argentina Observatorio Astronomico de la Universidad Nacional de Cordoba - Argentina
2	Gamen, Roberto	Hombre	UNIV NACL LA PLATA - Argentina Instituto de Astrofísica de La Plata (CONICET- Universidad Nacional de La Plata) - Argentina Instituto de Astrofisica de La Plata - Argentina
3	van Hoof, Peter A. M.	Hombre	Royal Observ Belgium - Bélgica Royal Observatory of Belgium - Bélgica
3	van Hoof, Peter A.M.	-	Royal Observatory of Belgium - Bélgica
4	Zijlstra, Albert A.	Hombre	UNIV MANCHESTER - Reino Unido University of Manchester - Reino Unido The University of Manchester - Reino Unido
5	MINNITI-DEL BARCO, DANTE	Hombre	Pontificia Universidad Católica de Chile - Chile Vatican Observ - Vaticano Universidad Nacional Andrés Bello - Chile Centro de Excelencia en Astrofísica y Tecnologías Afines - Chile Vatican Observatory - Italia
6	Volpe, M. G.	-	Inst Astron Teor & Expt - Argentina Instituto de Astronomia Teorica y Experimental - Argentina

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Origen de Citas Identificadas

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Citas identificadas: Las citas provienen de documentos incluidos en la base de datos de DATACIENCIA

Citas Identificadas: 20.0 %
Citas No-identificadas: 80.0 %

Muestra la distribución de instituciones nacionales o extranjeras cuyos autores citan a la publicación consultada.

Citas identificadas: Las citas provienen de documentos incluidos en la base de datos de DATACIENCIA

Citas Identificadas: 20.0 %
Citas No-identificadas: 80.0 %

Financiamiento

Fuente
National Science Foundation
Fondo Nacional de Desarrollo Científico y Tecnológico
Comisión Nacional de Investigación Científica y Tecnológica
NSF
Universidad Católica
NASA
STFC
Science and Technology Facilities Council
National Aeronautics and Space Administration
Fondo de Financiamiento de Centros de Investigación en Áreas Prioritarias
Belgian Federal Science policy Office
European Space Agency
University of Massachusetts
BASAL CATA Center for Astrophysics and Associated Technologies
Belgian Science Policy Office through the ESA PRODEX program
FONDAP Center for Astrophysics
ESO Public Survey
MILENIO Milky Way Millennium Nucleus from the Ministry of Economy's ICM
Proyecto FONDECYT from CONICYT
astro-Enginiering center at the Universidad Catolica (AIUC)
Ministry of Economy’s ICM
AIUC

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Agradecimientos

Agradecimiento
We thank the anonymous referee whose very useful remarks helped us to substantially improve this paper. We acknowledge Jim Emerson for comments that helped to improve the paper. This research has made use of the Aladin and SIMBAD database, operated at CDS, Strasbourg, France. This publication makes use of data products from the Two Micron All Sky Survey, a joint Project of the University of Massachusetts and IPAC/CALTECH, funded by NASA and NSF. We gratefully acknowledge use of data from the ESO Public Survey programme ID 179.B-2002 taken with the VISTA telescope, data products from the Cambridge Astronomical Survey Unit (CASU), and from the VISTA Science Archive at the Wide Field Astronomy Unit (WFAU). P.v.H. acknowledges support from the Belgian Science Policy Office through the ESA PRODEX program. D.M. gratefully acknowledges funding from the FONDAP Center for Astrophysics 15010003, the BASAL CATA Center for Astrophysics and Associated Technologies PFB-06, the MILENIO Milky Way Millennium Nucleus from the Ministry of Economy's ICM grant P07-021-F, and Proyecto FONDECYT Regular No. 1090213 from CONICYT and the astro-Enginiering center at the Universidad Catolica (AIUC).
We thank the anonymous referee whose very useful remarks helped us to substantially improve this paper. We acknowledge Jim Emerson for comments that helped to improve the paper. This research has made use of the Aladin and SIMBAD database, operated at CDS, Strasbourg, France. This publication makes use of data products from the Two Micron All Sky Survey, a joint Project of the University of Massachusetts and IPAC/CALTECH, funded by NASA and NSF. We gratefully acknowledge use of data from the ESO Public Survey programme ID 179.B-2002 taken with the VISTA telescope, data products from the Cambridge Astronomical Survey Unit (CASU), and from the VISTA Science Archive at the Wide Field Astronomy Unit (WFAU). P.v.H. acknowledges support from the Belgian Science Policy Office through the ESA PRODEX program. D.M. gratefully acknowledges funding from the FONDAP Center for Astrophysics 15010003, the BASAL CATA Center for Astrophysics and Associated Technologies PFB-06, the MILENIO Milky Way Millennium Nucleus from the Ministry of Economy’s ICM grant P07-021-F, and Proyecto FONDECYT Regular No. 1090213 from CONICYT and the astro-Enginiering center at the Universidad Católica (AIUC).

Agradecimiento

We thank the anonymous referee whose very useful remarks helped us to substantially improve this paper. We acknowledge Jim Emerson for comments that helped to improve the paper. This research has made use of the Aladin and SIMBAD database, operated at CDS, Strasbourg, France. This publication makes use of data products from the Two Micron All Sky Survey, a joint Project of the University of Massachusetts and IPAC/CALTECH, funded by NASA and NSF. We gratefully acknowledge use of data from the ESO Public Survey programme ID 179.B-2002 taken with the VISTA telescope, data products from the Cambridge Astronomical Survey Unit (CASU), and from the VISTA Science Archive at the Wide Field Astronomy Unit (WFAU). P.v.H. acknowledges support from the Belgian Science Policy Office through the ESA PRODEX program. D.M. gratefully acknowledges funding from the FONDAP Center for Astrophysics 15010003, the BASAL CATA Center for Astrophysics and Associated Technologies PFB-06, the MILENIO Milky Way Millennium Nucleus from the Ministry of Economy's ICM grant P07-021-F, and Proyecto FONDECYT Regular No. 1090213 from CONICYT and the astro-Enginiering center at the Universidad Catolica (AIUC).

We thank the anonymous referee whose very useful remarks helped us to substantially improve this paper. We acknowledge Jim Emerson for comments that helped to improve the paper. This research has made use of the Aladin and SIMBAD database, operated at CDS, Strasbourg, France. This publication makes use of data products from the Two Micron All Sky Survey, a joint Project of the University of Massachusetts and IPAC/CALTECH, funded by NASA and NSF. We gratefully acknowledge use of data from the ESO Public Survey programme ID 179.B-2002 taken with the VISTA telescope, data products from the Cambridge Astronomical Survey Unit (CASU), and from the VISTA Science Archive at the Wide Field Astronomy Unit (WFAU). P.v.H. acknowledges support from the Belgian Science Policy Office through the ESA PRODEX program. D.M. gratefully acknowledges funding from the FONDAP Center for Astrophysics 15010003, the BASAL CATA Center for Astrophysics and Associated Technologies PFB-06, the MILENIO Milky Way Millennium Nucleus from the Ministry of Economy’s ICM grant P07-021-F, and Proyecto FONDECYT Regular No. 1090213 from CONICYT and the astro-Enginiering center at the Universidad Católica (AIUC).

Muestra la fuente de financiamiento declarada en la publicación.

Abstract

Revista

Métricas Externas

Disciplinas de Investigación

Colaboración Institucional

Autores - Afiliación

Origen de Citas Identificadas

Financiamiento

Agradecimientos

Departamento Gestión de Conocimiento, Monitoreo y Prospección