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Article: VISTA Variables in the Vía Láctea (VVV): Current Status and First Results

TitleVISTA Variables in the Vía Láctea (VVV): Current Status and First Results
Authors
Saito, RHempel, MAlonso-García, JToledo, IBorissova, JGonzález, OBeamin, JCMinniti, DLucas, PEmerson, JAhumada, AAigrain, SAlonso, MVAmôres, EAngeloni, RArias, JBandyopadhyay, RBarbá, RBarbuy, BBaume, GBedin, LBica, EBronfman, LCarraro, GCatelan, MClariá, JContreras, CCross, NDavis, Cde Grijs, RDékány, IJanet Drew, JDFariña, CFeinstein, CFernández LEFolkes, SGamen, RGeisler, DGieren, WGoldman, BGosling, AGunthardt, GGurovich, SHambly, NHanson, MHoare, MIrwin, MIvanov, VJordán, AKerins, EKinemuchi, KKurtev, RLongmore, ALópez-Corredoira, MMaccarone, TMartín, EMasetti, NMennickent, RMerlo, DMessineo, MMirabel, FMonaco, LMoni Bidin, CMorelli, LPadilla, NPalma, TParisi, MCParker, QAPavani, DPietrukowicz, PPietrzynski, GPignata, GRejkuba, MRojas, ARoman LARuiz, MTSale, SSaviane, ISchreiber, MSchröder, ASharma, SSmith, MSodré, L JrSoto, MStephens, ATamura, MTappert, CThompson, MValenti, EVanzi, LWeidmann, WZoccali, M
Issue Date2010
Citation
The Messenger, 2010, v. 141, p. 24-28 How to Cite?
AbstractVISTA Variables in the Vía Láctea (VVV) is a public ESO near-IR variability survey aimed at scanning the Milky Way Bulge and an adjacent section of the mid-plane. VVV observations started in October 2009 during ESO science verification. Regular observations for the first year of the survey have been conducted since February 2010 and will cover a total area of 520 square degrees in five passbands and five epochs. Here we address the first results obtained from the VVV Survey as well as the current status of the observations.
Persistent Identifierhttp://hdl.handle.net/10722/211295
ISSN
0722-6691

 

DC FieldValueLanguage
dc.contributor.authorSaito, R-
dc.contributor.authorHempel, M-
dc.contributor.authorAlonso-García, J-
dc.contributor.authorToledo, I-
dc.contributor.authorBorissova, J-
dc.contributor.authorGonzález, O-
dc.contributor.authorBeamin, JC-
dc.contributor.authorMinniti, D-
dc.contributor.authorLucas, P-
dc.contributor.authorEmerson, J-
dc.contributor.authorAhumada, A-
dc.contributor.authorAigrain, S-
dc.contributor.authorAlonso, MV-
dc.contributor.authorAmôres, E-
dc.contributor.authorAngeloni, R-
dc.contributor.authorArias, J-
dc.contributor.authorBandyopadhyay, R-
dc.contributor.authorBarbá, R-
dc.contributor.authorBarbuy, B-
dc.contributor.authorBaume, G-
dc.contributor.authorBedin, L-
dc.contributor.authorBica, E-
dc.contributor.authorBronfman, L-
dc.contributor.authorCarraro, G-
dc.contributor.authorCatelan, M-
dc.contributor.authorClariá, J-
dc.contributor.authorContreras, C-
dc.contributor.authorCross, N-
dc.contributor.authorDavis, C-
dc.contributor.authorde Grijs, R-
dc.contributor.authorDékány, I-
dc.contributor.authorJanet Drew, JD-
dc.contributor.authorFariña, C-
dc.contributor.authorFeinstein, C-
dc.contributor.authorFernández LE-
dc.contributor.authorFolkes, S-
dc.contributor.authorGamen, R-
dc.contributor.authorGeisler, D-
dc.contributor.authorGieren, W-
dc.contributor.authorGoldman, B-
dc.contributor.authorGosling, A-
dc.contributor.authorGunthardt, G-
dc.contributor.authorGurovich, S-
dc.contributor.authorHambly, N-
dc.contributor.authorHanson, M-
dc.contributor.authorHoare, M-
dc.contributor.authorIrwin, M-
dc.contributor.authorIvanov, V-
dc.contributor.authorJordán, A-
dc.contributor.authorKerins, E-
dc.contributor.authorKinemuchi, K-
dc.contributor.authorKurtev, R-
dc.contributor.authorLongmore, A-
dc.contributor.authorLópez-Corredoira, M-
dc.contributor.authorMaccarone, T-
dc.contributor.authorMartín, E-
dc.contributor.authorMasetti, N-
dc.contributor.authorMennickent, R-
dc.contributor.authorMerlo, D-
dc.contributor.authorMessineo, M-
dc.contributor.authorMirabel, F-
dc.contributor.authorMonaco, L-
dc.contributor.authorMoni Bidin, C-
dc.contributor.authorMorelli, L-
dc.contributor.authorPadilla, N-
dc.contributor.authorPalma, T-
dc.contributor.authorParisi, MC-
dc.contributor.authorParker, QA-
dc.contributor.authorPavani, D-
dc.contributor.authorPietrukowicz, P-
dc.contributor.authorPietrzynski, G-
dc.contributor.authorPignata, G-
dc.contributor.authorRejkuba, M-
dc.contributor.authorRojas, A-
dc.contributor.authorRoman LA-
dc.contributor.authorRuiz, MT-
dc.contributor.authorSale, S-
dc.contributor.authorSaviane, I-
dc.contributor.authorSchreiber, M-
dc.contributor.authorSchröder, A-
dc.contributor.authorSharma, S-
dc.contributor.authorSmith, M-
dc.contributor.authorSodré, L Jr-
dc.contributor.authorSoto, M-
dc.contributor.authorStephens, A-
dc.contributor.authorTamura, M-
dc.contributor.authorTappert, C-
dc.contributor.authorThompson, M-
dc.contributor.authorValenti, E-
dc.contributor.authorVanzi, L-
dc.contributor.authorWeidmann, W-
dc.contributor.authorZoccali, M-
dc.date.accessioned2015-07-08T03:24:18Z-
dc.date.available2015-07-08T03:24:18Z-
dc.date.issued2010-
dc.identifier.citationThe Messenger, 2010, v. 141, p. 24-28-
dc.identifier.issn0722-6691-
dc.identifier.urihttp://hdl.handle.net/10722/211295-
dc.description.abstractVISTA Variables in the Vía Láctea (VVV) is a public ESO near-IR variability survey aimed at scanning the Milky Way Bulge and an adjacent section of the mid-plane. VVV observations started in October 2009 during ESO science verification. Regular observations for the first year of the survey have been conducted since February 2010 and will cover a total area of 520 square degrees in five passbands and five epochs. Here we address the first results obtained from the VVV Survey as well as the current status of the observations.-
dc.languageeng-
dc.relation.ispartofThe Messenger-
dc.titleVISTA Variables in the Vía Láctea (VVV): Current Status and First Results-
dc.typeArticle-
dc.identifier.emailParker, QA: quentinp@hku.hk-
dc.identifier.authorityParker, QA=rp02017-
dc.identifier.volume141-
dc.identifier.spage24-
dc.identifier.epage28-
dc.identifier.issnl0722-6691-

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