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dc.creatorMinniti, D.
dc.creatorSaito, R.
dc.creatorHempel, M.
dc.creatorBarbá, R.11Bronfman, L.
dc.creatorCatelan, M.
dc.creatorGeisler, D.
dc.creatorGieren, W.
dc.creatorJordan, A.
dc.creatorMonaco, L.
dc.creatorPadilla, N.
dc.creatorPignata, G.
dc.creatorZoccali, M.
dc.creatorPietrzynski, G.
dc.date.accessioned2020-03-11T20:35:52Z
dc.date.available2020-03-11T20:35:52Z
dc.date.issued2010
dc.identifier.urihttp://hdl.handle.net/10533/240769
dc.description.abstractWe describe the public ESO near-IR variability survey (VVV) scanning the Milky Way bulge and an adjacent section of the mid-plane where star formation activity is high. The survey will take 1929 h of observations with the 4-m VISTA telescope during 5 year
dc.language.isoeng
dc.relation.urihttps://doi.org/10.1016/j.newast.2009.12.002
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.titleVISTA Variables in the Via Lactea (VVV): The public ESO near-IR variability survey of the Milky Way
dc.typeArticulo
dc.identifier.folio15010003
dc.description.conicytprogramFONDAP
dc.rights.driverinfo:eu-repo/semantics/openAccess
dc.title.journalNew Astronomy
dc.type.driverinfo:eu-repo/semantics/article
dc.description.shortconicytprogramFONDAP
dc.type.openaireinfo:eu-repo/semantics/publishedVersion


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