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Article: The VVV Survey of the Milky Way: first year results

TitleThe VVV Survey of the Milky Way: first year results
Authors
Issue Date2011
Citation
Boletin de la Asociacion Argentina de Astronomia La Plata Argentina, 2011, v. 54, p. 265-276 How to Cite?
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.
Persistent Identifierhttp://hdl.handle.net/10722/211294
ISSN

 

DC FieldValueLanguage
dc.contributor.authorMinniti, D-
dc.contributor.authorClariá, JJ-
dc.contributor.authorSaito, RK-
dc.contributor.authorHempel, M-
dc.contributor.authorLucas, PW-
dc.contributor.authorRejkuba, M-
dc.contributor.authorToledo, I-
dc.contributor.authorGonzalez, OA-
dc.contributor.authorAlonso-García, J-
dc.contributor.authorIrwin, MJ-
dc.contributor.authorGonzalez-Solares, E-
dc.contributor.authorCross, N-
dc.contributor.authorIvanov, VD-
dc.contributor.authorSoto, M-
dc.contributor.authorDékány, I-
dc.contributor.authorAngeloni, R-
dc.contributor.authorCatelan, M-
dc.contributor.authorAmôres, EB-
dc.contributor.authorGurovich, S-
dc.contributor.authorEmerson, JP-
dc.contributor.authorLewis, J-
dc.contributor.authorHodgkin, S-
dc.contributor.authorPietrukowicz, P-
dc.contributor.authorZoccali, M-
dc.contributor.authorSale, SE-
dc.contributor.authorBarbá, R-
dc.contributor.authorBarbuy, B-
dc.contributor.authorBeamin, JC-
dc.contributor.authorHelminiak, K-
dc.contributor.authorBorissova, J-
dc.contributor.authorFolkes, SL-
dc.contributor.authorGamen, RC-
dc.contributor.authorGeisler, D-
dc.contributor.authorMauro, F-
dc.contributor.authorChené, AN-
dc.contributor.authorAlonso, MV-
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, IF-
dc.contributor.authorMonaco, L-
dc.contributor.authorMoni BC-
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, AV-
dc.contributor.authorAigrain, S-
dc.contributor.authorArias, JI-
dc.contributor.authorBica, E-
dc.contributor.authorBandyopadhyay, RM-
dc.contributor.authorBaume, G-
dc.contributor.authorBedin, LR-
dc.contributor.authorBonatto, C-
dc.contributor.authorBronfman, L-
dc.contributor.authorCarraro, G-
dc.contributor.authorContreras, C-
dc.contributor.authorDavis, CJ-
dc.contributor.authorde Grijs, R-
dc.contributor.authorDias, B-
dc.contributor.authorDrew, JE-
dc.contributor.authorFariña, C-
dc.contributor.authorFeinstein, C-
dc.contributor.authorFernández LE-
dc.contributor.authorGieren, W-
dc.contributor.authorGoldman, B-
dc.contributor.authorGosling, A-
dc.contributor.authorHambly, NC-
dc.contributor.authorHoare, M-
dc.contributor.authorJordán, A-
dc.contributor.authorKinemuchi, K-
dc.contributor.authorMaccarone, T-
dc.contributor.authorMerlo, DC-
dc.contributor.authorMennickent, RE-
dc.contributor.authorMorelli, L-
dc.contributor.authorMotta, V-
dc.contributor.authorPalma, T-
dc.contributor.authorPopescu, B-
dc.contributor.authorParisi, MC-
dc.contributor.authorParker, QA-
dc.contributor.authorPignata, G-
dc.contributor.authorRead, MA-
dc.contributor.authorRuiz, MT-
dc.contributor.authorRoman-Lopes, A-
dc.contributor.authorSchreiber, MR-
dc.contributor.authorSchröder, AC-
dc.contributor.authorSmith, M-
dc.contributor.authorSodré, L Jr-
dc.contributor.authorStephens, AA-
dc.contributor.authorWalton, NA-
dc.contributor.authorZijlstra, AA-
dc.contributor.authorTamura, M-
dc.contributor.authorTappert, C-
dc.contributor.authorThompson, MA-
dc.contributor.authorVanzi, L-
dc.date.accessioned2015-07-08T03:24:17Z-
dc.date.available2015-07-08T03:24:17Z-
dc.date.issued2011-
dc.identifier.citationBoletin de la Asociacion Argentina de Astronomia La Plata Argentina, 2011, v. 54, p. 265-276-
dc.identifier.issn0571-3285-
dc.identifier.urihttp://hdl.handle.net/10722/211294-
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.languageeng-
dc.relation.ispartofBoletin de la Asociacion Argentina de Astronomia La Plata Argentina-
dc.titleThe VVV Survey of the Milky Way: first year results-
dc.typeArticle-
dc.identifier.emailParker, QA: quentinp@hku.hk-
dc.identifier.authorityParker, QA=rp02017-
dc.identifier.volume54-
dc.identifier.spage265-
dc.identifier.epage276-

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