Stellar variability in the VVV survey

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dc.contributor.authorCatelan, Márcio
dc.contributor.authorMinniti, D.
dc.contributor.authorLucas, P. W.
dc.contributor.authorDékány, I.
dc.contributor.authorSaito, R. K.
dc.contributor.authorAngeloni, Rodolfo
dc.contributor.authorAlonso-García, J.
dc.contributor.authorHempel, M.
dc.contributor.authorHelminiak, Krzysztof Grzegorz
dc.contributor.authorJordán, A.
dc.contributor.authorContreras Ramos, Rodrigo Andrés
dc.contributor.authorNavarrete, C.
dc.contributor.authorBeamin Muhlenbrock, Juan Carlos
dc.contributor.authorRojas, A. F.
dc.contributor.authorGran, F.
dc.contributor.authorFerreira Lopes, C. E.
dc.contributor.author Contreras Peña, Carlos Eduardo
dc.contributor.authorKerins, E.
dc.contributor.authorHuckvale, L.
dc.contributor.authorRejkuba, M.
dc.contributor.authorCohen, R.
dc.contributor.authorMauro, F.
dc.contributor.authorBorissova, J.
dc.contributor.authorAmigo, P.
dc.contributor.authorEyheramendy Duerr, Susana
dc.contributor.authorPichara Baksai, Karim Elías
dc.contributor.authorEspinoza, N.
dc.contributor.authorNavarro, C.
dc.contributor.authorHajdu, G.
dc.contributor.authorCalderón Espinoza, Diego Nicolás
dc.contributor.authorMuro, G. A.
dc.contributor.authorAndrews, H.
dc.contributor.authorMotta, V.
dc.contributor.authorKurtev, R.
dc.contributor.authorEmerson, J. P.
dc.contributor.authorMoni Bidin, C.
dc.contributor.authorChené, A. -N.
dc.date.accessioned2020-05-07T21:05:54Z
dc.date.available2020-05-07T21:05:54Z
dc.date.issued2013
dc.date.updated2020-05-07T19:57:31Z
dc.description.abstractThe Vista Variables in the Via Lactea (VVV) ESO Public Survey is an ongoing time-series, near-infrared (IR) survey of the Galactic bulge and an adjacent portion of the inner disk, covering 562 square degrees of the sky, using ESOs VISTA telescope. The survey has provided superb multi-color photometry in 5 broadband filters ($Z$, $Y$, $J$, $H$, and $K_s$), leading to the best map of the inner Milky Way ever obtained, particularly in the near-IR. The main variability part of the survey, which is focused on $K_s$-band observations, is currently underway, with bulge fields having been observed between 31 and 70 times, and disk fields between 17 and 36 times. When the survey is complete, bulge (disk) fields will have been observed up to a total of 100 (60) times, providing unprecedented depth and time coverage. Here we provide a first overview of stellar variability in the VVV data, including examples of the light curves that have been collected thus far, scientific applications, and our efforts towards the automated classification of VVV light curves....
dc.identifier.urihttps://arxiv.org/abs/1310.1996
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/28880
dc.language.isoen
dc.revistaarXiv e-printses_ES
dc.rightsacceso abierto
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.subject.otherEstrellas -- Observacioneses_ES
dc.subject.otherEstrellas variables - Catálogoses_ES
dc.subject.otherGalaxiaes_ES
dc.titleStellar variability in the VVV surveyes_ES
dc.typeartículo
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