Maria-Rosa L. Cioni, the VMC team
Published 2015-03-24Version 1
The VISTA survey of the Magellanic Clouds system (VMC) is a public survey project of the European Southern Observatory. It is collecting multi-band near-infrared data across large areas of the Large and Small Magellanic Clouds, the Magellanic Bridge and a few fields in the Magellanic Stream. The combination of great sensitivity to stars below the old main sequence turn off, and the multiplicity at Ks band (at least 12 epochs) make VMC highly suitable for the determination of the spatially resolved star formation history and three-dimensional geometry, using variable stars such as Cepheids and RR Lyrae stars. The VMC observations are progressing well and will be completed in 2018. The VMC survey has a high legacy value and many science results have already been published, e.g. the most detailed star formation history map of the Small Magellanic Cloud, and others are in preparation, e.g. a comprehensive investigation of classical Cepheids and a study of the proper motion in the foreground 47 Tuc cluster.
Comments: 5 pages, 1 figure, Proceeding contribution of targeted talk at the conference "The Universe of Digital Sky Surveys" held in Naples (Italy) on 25-28 November 2014
The VMC Survey - XXI. New star cluster candidates discovered from infrared photometry in the Small Magellanic Cloud
The VMC Survey. XXVIII. The 3D structure of the Small Magellanic Cloud from Classical Cepheids
The VMC survey -- XXXIX: Mapping metallicity trends in the Small Magellanic Cloud using near-infrared passbands
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