Stellar Variability in the VVV Survey: An Update

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dc.catalogadormas
dc.contributor.authorCatelan, Marcio
dc.contributor.authorDekany, I.
dc.contributor.authorHempel, M.
dc.contributor.authorMinniti, D.
dc.date.accessioned2024-02-02T13:58:49Z
dc.date.available2024-02-02T13:58:49Z
dc.date.issued2014
dc.description.abstractThe Vista Variables in the Via Lactea (VVV) ESO Public Survey consists in a near-infrared time-series survey of the Galactic bulge and inner disk, covering 562 square degrees of the sky, over a total timespan of more than 5 years. In this paper, we provide an updated account of the current status of the survey, especially in the context of stellar variability studies. In this sense, we give a first description of our efforts towards the construction of the VVV Variable Star Catalog (VVV-VSC)....
dc.fuente.origenORCID
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/81299
dc.information.autorucInstituto de Astrofísica; Catelan , Marcio; 0000-0001-6003-8877; 1001556
dc.language.isoen
dc.nota.accesocontenido parcial
dc.rightsacceso restringido
dc.titleStellar Variability in the VVV Survey: An Update
dc.typedocumento de trabajo
sipa.codpersvinculados1001556
sipa.trazabilidadORCID;2024-01-22
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