VISTA Milky Way Public Survey

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dc.catalogadorpau
dc.contributor.authorMinniti, D.
dc.contributor.authorLucas, P.
dc.contributor.authorAhumada, A. V.
dc.contributor.authorZoccali, M.
dc.contributor.authorCatelan, Marcio
dc.contributor.authorMorelli, L.
dc.contributor.authorTappert, C.
dc.contributor.authorPignata, G.
dc.contributor.authorToledo, I.
dc.contributor.authorRuiz, M. T.
dc.contributor.authorCarraro, G.
dc.contributor.authorCasassus, S.
dc.contributor.authorBronfman, L.
dc.contributor.authorBarbá, R. H.
dc.contributor.authorGamen, R.
dc.contributor.authorGieren, W.
dc.contributor.authorGeisler, D.
dc.contributor.authorPietrzynski, G.
dc.contributor.authorMennickent, R. E.
dc.contributor.authorKurtev, R.
dc.contributor.authorBorissova, J.
dc.contributor.authorMirabel, F.
dc.contributor.authorIvanov, V. D.
dc.contributor.authorSaviane, I.
dc.contributor.authorVanzi, L.
dc.contributor.authorMonaco, L.
dc.contributor.authorRejkuba, M.
dc.contributor.authorMessineo, M.
dc.contributor.authorBedin, L.
dc.contributor.authorStephens, A.
dc.contributor.authorBarbuy, B.
dc.contributor.authorBica, E.
dc.contributor.authorClariá, J. J.
dc.contributor.authorCASU (VDFS) Team
dc.contributor.authorWFAU (VDFS) Team
dc.contributor.authorEmerson, J.
dc.contributor.authorDrew, J.
dc.contributor.authorLópez-Correidora, M.
dc.contributor.authorMartin, E.
dc.contributor.authorGoldman, B.
dc.contributor.authorGianinni, T.
dc.contributor.authorEisloeffel, J.
dc.contributor.authorGroot, P.
dc.contributor.authorFabregat, J.
dc.contributor.authorHambly, N.
dc.contributor.authorLongmore, A.
dc.contributor.authorWalton, N.
dc.contributor.authorde Grijs, R.
dc.contributor.authorHoare, M.
dc.contributor.authorSchroeder, A.
dc.contributor.authorNaylor, T.
dc.contributor.authorBarlow, M.
dc.contributor.authorZijlstra, A.
dc.contributor.authorWhite, G.
dc.contributor.authorGosling, A.
dc.contributor.authorMcGowan, K.
dc.contributor.authorAdamson, A.
dc.contributor.authorBandyopadhyay, R.
dc.contributor.authorThompson, M.
dc.contributor.authorCropper, M.
dc.contributor.authorLucey, J.
dc.contributor.authorKerins, E.
dc.contributor.authorHodgkin, S.
dc.contributor.authorPinfield, D.
dc.date.accessioned2024-03-05T15:15:07Z
dc.date.available2024-03-05T15:15:07Z
dc.date.issued2009
dc.description.abstractWe propose a public IR variability survey, named ``Vista Variables in the Vía Láctea'' (VVV), of the Milky Way bulge and an adjacent section of the mid-plane where star formation activity is high. This would take 1920 hours, covering ∼ 10^9 point sources within an area of 520 sq deg, including 33 known globular clusters and ∼ 350 open clusters. The final products will be a deep IR atlas in 5 passbands and a catalogue of ∼ 10^6 variable point sources. These will produce a 3-D map of the surveyed region (unlike single-epoch surveys that only give 2-D maps) using well-understood primary distance indicators such as RR Lyrae stars. It will yield important information on the ages of the populations. The observations will be combined with data from MACHO, OGLE, EROS, VST, SPITZER, HST, CHANDRA, INTEGRAL, and ALMA for a complete understanding of the variable sources in the inner Milky Way. Several important implications for the history of the Milky Way, for globular cluster evolution, for the population census of the bulge and center, and for pulsation theory would follow from this survey....
dc.fechaingreso.objetodigital2024-05-17
dc.fuente.origenORCID
dc.identifier.urihttps://www.redalyc.org/articulo.oa?id=57115758102
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/84113
dc.information.autorucInstituto de Astrofísica; Catelan , Marcio; 0000-0001-6003-8877; 1001556
dc.language.isoen
dc.nota.accesoContenido completo
dc.rightsacceso abierto
dc.titleVISTA Milky Way Public Survey
dc.typecomunicación de congreso
sipa.codpersvinculados1001556
sipa.trazabilidadORCID;2024-01-22
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