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  • VISTA Variables in the V\'ia L\'actea (VVV): Halfway Status and Results
    Hempel, Maren; Minniti, Dante; Dékány, István; Saito, Roberto K; Lucas, Philip W; Emerson, Jim; Ahumada, Andrea V; Aigrain, Suzanne; Alonso, Maria Victoria; Alonso-García, Javier; Amôres, Eduardo B; Angeloni, Rodolfo; Arias, Julia; Bandyopadhyay, Reba; Barbá, Rodolfo H; Barbuy, Beatriz; Baume, Gustavo; Beamin, Juan Carlos; Bedin, Luigi; Bica, Eduardo; Borissova, Jordanka; Bronfman, Leonardo; Carraro, Giovanni; Catelan, Márcio; Clariá, Juan J; Contreras, Carlos; Cross, Nicholas; Davis, Christopher; de Grijs, Richard; Drew, Janet E; Fariña, Cecilia; Feinstein, Carlos; Lajús, Eduardo Fernández; Folkes, Stuart; Gamen, Roberto C; Geisler, Douglas; Gieren, Wolfgang; Goldman, Bertrand; González, Oscar; Gosling, Andrew; Gunthardt, Guillermo; Gurovich, Sebastian; Hambly, Nigel C; Hanson, Margaret; Hoare, Melvin; Irwin, Mike J; Ivanov, Valentin D; Jordán, Andrés; Kerins, Eamonn; Kinemuchi, Karen; Kurtev, Radostin; Longmore, Andy; López-Corredoira, Martin; Maccarone, Tom; Martín, Eduardo; Masetti, Nicola; Mennickent, Ronald E; Merlo, David; Messineo, Maria; Mirabel, I. Félix; Monaco, Lorenzo; Bidin, Christian Moni; Morelli, Lorenzo; Padilla, Nelson; Palma, Tali; Parisi, Maria Celeste; Parker, Quentin; Pavani, Daniela; Pietrukowicz, Pawel; Pietrzynski, Grzegorz; Pignata, Giuliano; Rejkuba, Marina; Rojas, Alejandra; Roman-Lopes, Alexandre; Ruiz, Maria Teresa; Sale, Stuart E; Saviane, Ivo; Schreiber, Matthias R; Schröder, Anja C; Sharma, Saurabh; Smith, Michael; SodréJr, Laerte; Soto, Mario; Stephens, Andrew W; Tamura, Motohide; Tappert, Claus; Thompson, Mark A; Toledo, Ignacio; Valenti, Elena; Vanzi, Leonardo; Weidmann, Walter; Zoccali, Manuela

    06/2014
    Journal Article

    ESO Messenger 155, (2014), 29-32 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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