The VVV Survey of the Milky Way: first year results

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dc.catalogadorpau
dc.contributor.authorMinniti, D.
dc.contributor.authorClariá, J. J.
dc.contributor.authorSaito, R. K.
dc.contributor.authorHempel, M.
dc.contributor.authorLucas, P. W.
dc.contributor.authorRejkuba, M.
dc.contributor.authorToledo, I.
dc.contributor.authorGonzalez, O. A.
dc.contributor.authorAlonso-García, J.
dc.contributor.authorIrwin, M. J.
dc.contributor.authorGonzalez-Solares, E.
dc.contributor.authorCross, N.
dc.contributor.authorIvanov, V. D.
dc.contributor.authorSoto, M.
dc.contributor.authorDékány, I.
dc.contributor.authorAngeloni, R.
dc.contributor.authorCatelan, Marcio
dc.contributor.authorAmôres, E. B.
dc.contributor.authorGurovich, S.
dc.contributor.authorEmerson, J. P.
dc.contributor.authorLewis, J.
dc.contributor.authorHodgkin, S.
dc.contributor.authorPietrukowicz, P.
dc.contributor.authorZoccali, M.
dc.contributor.authorSale, S. E.
dc.contributor.authorBarbá, R.
dc.contributor.authorBarbuy, B.
dc.contributor.authorBeamin, J. C.
dc.contributor.authorHelminiak, K.
dc.contributor.authorBorissova, J.
dc.contributor.authorFolkes, S. L.
dc.contributor.authorGamen, R. C.
dc.contributor.authorGeisler, D.
dc.contributor.authorMauro, F.
dc.contributor.authorChené, A. -N.
dc.contributor.authorAlonso, M. V.
dc.contributor.authorGunthardt, G.
dc.contributor.authorHanson, M.
dc.contributor.authorKerins, E.
dc.contributor.authorKurtev, R.
dc.contributor.authorMajaess, D.
dc.contributor.authorMartín, E.
dc.contributor.authorMasetti, N.
dc.contributor.authorMirabel, I. F.
dc.contributor.authorMonaco, L.
dc.contributor.authorMoni Bidin, C.
dc.contributor.authorPadilla, N.
dc.contributor.authorRojas, A.
dc.contributor.authorPietrzynski, G.
dc.contributor.authorSaviane, I.
dc.contributor.authorValenti, E.
dc.contributor.authorWeidmann, W.
dc.contributor.authorLópez-Corredoira, M.
dc.contributor.authorAhumada, A. V.
dc.contributor.authorAigrain, S.
dc.contributor.authorArias, J. I.
dc.contributor.authorBica, E.
dc.contributor.authorBandyopadhyay, R. M.
dc.contributor.authorBaume, G.
dc.contributor.authorBedin, L. R.
dc.contributor.authorBonatto, C.
dc.contributor.authorBronfman, L.
dc.contributor.authorCarraro, G.
dc.contributor.authorContreras, C.
dc.contributor.authorDavis, C. J.
dc.contributor.authorde Grijs, R.
dc.contributor.authorDias, B.
dc.contributor.authorDrew, J. E.
dc.contributor.authorFariña, C.
dc.contributor.authorFeinstein, C.
dc.contributor.authorFernández Lajús, E.
dc.contributor.authorGieren, W.
dc.contributor.authorGoldman, B.
dc.contributor.authorGosling, A.
dc.contributor.authorHambly, N. C.
dc.contributor.authorHoare, M.
dc.contributor.authorJordán, A.
dc.contributor.authorKinemuchi, K.
dc.contributor.authorMaccarone, T.
dc.contributor.authorMerlo, D. C.
dc.contributor.authorMennickent, R. E.
dc.contributor.authorMorelli, L.
dc.contributor.authorMotta, V.
dc.contributor.authorPalma, T.
dc.contributor.authorPopescu, B.
dc.contributor.authorParisi, M. C.
dc.contributor.authorParker, Q.
dc.contributor.authorPignata, G.
dc.contributor.authorRead, M. A.
dc.contributor.authorRuiz, M. T.
dc.contributor.authorRoman-Lopes, A.
dc.contributor.authorSchreiber, M. R.
dc.contributor.authorSchröder, A. C.
dc.contributor.authorSmith, M.
dc.contributor.authorSodré, L., Jr.
dc.contributor.authorStephens, A. W.
dc.contributor.authorWalton, N. A.
dc.contributor.authorZijlstra, A. A.
dc.contributor.authorTamura, M.
dc.contributor.authorTappert, C.
dc.contributor.authorThompson, M. A.
dc.contributor.authorVanzi, L.
dc.date.accessioned2024-03-05T15:14:40Z
dc.date.available2024-03-05T15:14:40Z
dc.date.issued2011
dc.description.abstractThe VISTA Variables in the Via Lactea (VVV) is an ESO public near-IR variability survey that is scanning the Milky Way bulge and an adjacent section of the Galactic mid-plane. The survey will take 1929 hours of observations with the VISTA 4.1-m telescope during five years, covering a billion point sources across an area of 520 sqdeg, including 36 known globular clusters and more than 350 open clusters. The final product will be a deep IR atlas in five passbands (0.9 - 2.5 microns) and a catalogue of more than a million variable point sources....
dc.fuente.origenORCID
dc.identifier.urihttps://ui.adsabs.harvard.edu/abs/2011BAAA...54..265M/abstract
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/84001
dc.information.autorucInstituto de Astrofísica; Catelan , Marcio; 0000-0001-6003-8877; 1001556
dc.language.isoen
dc.rightsacceso abierto
dc.titleThe VVV Survey of the Milky Way: first year results
dc.typeartículo
sipa.codpersvinculados1001556
sipa.trazabilidadORCID;2024-01-22
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