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arxiv: 1406.3241 · v1 · pith:IFLYZ2QRnew · submitted 2014-06-12 · 🌌 astro-ph.IM

VISTA Variables in the V\'ia L\'actea (VVV): Halfway Status and Results

Maren Hempel , Dante Minniti , Istv\'an D\'ek\'any , Roberto K. Saito , Philip W. Lucas , Jim Emerson , Andrea V. Ahumada , Suzanne Aigrain
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Maria Victoria Alonso Javier Alonso-Garc\'ia Eduardo B. Am\^ores Rodolfo Angeloni Julia Arias Reba Bandyopadhyay Rodolfo H. Barb\'a Beatriz Barbuy Gustavo Baume Juan Carlos Beamin Luigi Bedin Eduardo Bica Jordanka Borissova Leonardo Bronfman Giovanni Carraro M\'arcio Catelan Juan J. Clari\'a Carlos Contreras Nicholas Cross Christopher Davis Richard de Grijs Janet E. Drew Cecilia Fari\~na Carlos Feinstein Eduardo Fern\'andez Laj\'us Stuart Folkes Roberto C. Gamen Douglas Geisler Wolfgang Gieren Bertrand Goldman Oscar Gonz\'alez Andrew Gosling Guillermo Gunthardt Sebastian Gurovich Nigel C. Hambly Margaret Hanson Melvin Hoare Mike J. Irwin Valentin D. Ivanov Andr\'es Jord\'an Eamonn Kerins Karen Kinemuchi Radostin Kurtev Andy Longmore Martin L\'opez-Corredoira Tom Maccarone Eduardo Mart\'in Nicola Masetti Ronald E. Mennickent David Merlo Maria Messineo I. F\'elix Mirabel Lorenzo Monaco Christian Moni Bidin Lorenzo Morelli Nelson Padilla Tali Palma Maria Celeste Parisi Quentin Parker Daniela Pavani Pawel Pietrukowicz Grzegorz Pietrzynski Giuliano Pignata Marina Rejkuba Alejandra Rojas Alexandre Roman-Lopes Maria Teresa Ruiz Stuart E. Sale Ivo Saviane Matthias R. Schreiber Anja C. Schr\"oder Saurabh Sharma Michael Smith Laerte Sodr\'e Jr. Mario Soto Andrew W. Stephens Motohide Tamura Claus Tappert Mark A. Thompson Ignacio Toledo Elena Valenti Leonardo Vanzi Walter Weidmann Manuela Zoccali
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keywords resultssurveyvariablesacteaobservingsomestatusvista
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The VISTA Variables in the V\'ia L\'actea (VVV) survey is one of six public ESO surveys, and is now in its 4th year of observing. Although far from being complete, the VVV survey has already delivered many results, some directly connected to the intended science goals (detection of variables stars, microlensing events, new star clusters), others concerning more exotic objects, e.g. novae. Now, at the end of the fourth observing period, and comprising roughly 50% of the proposed observations, the actual status of the survey, as well some of the results based on the VVV data, are presented.

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