Stellar Variability in the VVV Survey: Highlights and Current Status

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dc.catalogadormas
dc.contributor.authorCatelan, Marcio
dc.contributor.authorDékány, István
dc.contributor.authorMinniti, Dante
dc.contributor.authorAlonso-Garcia, Javier
dc.contributor.authorContreras Ramos, Rodrigo
dc.contributor.authorSaito, Roberto
dc.contributor.authorHajdu, Gergely
dc.contributor.authorLucas, Phil
dc.contributor.authorKerins, Eamonn
dc.contributor.authorHempel, Maren
dc.date.accessioned2024-02-02T13:58:48Z
dc.date.available2024-02-02T13:58:48Z
dc.date.issued2015
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 contribution, we discuss some of our latest results, and provide an updated account of the current status of the survey, especially in the context of stellar variability studies....
dc.fuente.origenORCID
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/81296
dc.information.autorucInstituto de Astrofísica; Catelan , Marcio; 0000-0001-6003-8877; 1001556
dc.language.isoen
dc.rightsregistro bibliográfico
dc.titleStellar Variability in the VVV Survey: Highlights and Current Status
dc.typecontribución de congreso
sipa.codpersvinculados1001556
sipa.trazabilidadORCID;2024-01-22
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