Vista variables in the via lactea (VVV): first results and perspectives

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dc.catalogadorvzp
dc.contributor.authorSaito, R. K.
dc.contributor.authorMinniti, D.
dc.contributor.authorDekany, I.
dc.contributor.authorHempel, M.
dc.contributor.authorAlonso-Garcia, J.
dc.contributor.authorToledo, I.
dc.contributor.authorBeamin Muhlenbrock, Juan Carlos
dc.contributor.authorAngeloni, R.
dc.contributor.authorLucas, P. W.
dc.contributor.authorEmerson, J. P.
dc.date.accessioned2024-03-15T16:02:45Z
dc.date.available2024-03-15T16:02:45Z
dc.date.issued2011
dc.description.abstractVISTA Variables in the Via Lactea (VVV) is a public ESO near-IR variability survey scanning the Milky Way Bulge and an adjacent section of the mid-plane. The survey will take 1929 hours of observations with the 4 m VISTA telescope during five years (2010-2014), covering similar to 10(9) point sources across an area of 520 deg(2). Here we address the first results obtained from the VVV Survey as well as a glimpse into the possibilities for using a deep near-IR atlas in five passbands and a catalogue of more than 10(6) variable point sources. We expect to use the data to find planetary transits of late-type main-sequence stars. We discuss the planet searches and future follow-ups
dc.fuente.origenORCID
dc.identifier.urihttps://publons.com/wos-op/publon/9906278/
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/84549
dc.information.autorucInstituto de Física; Beamin Muhlenbrock, Juan Carlos; 0000-0002-8409-6534; 154617
dc.language.isoen
dc.nota.accesoContenido parcial
dc.rightsacceso restringido
dc.subject.ddc520
dc.subject.deweyAstronomía
dc.titleVista variables in the via lactea (VVV): first results and perspectives
dc.typecomunicación de congreso
sipa.codpersvinculados154617
sipa.trazabilidadORCID;2024-03-11
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