TL;DR
The VMC survey is a comprehensive near-infrared observational project mapping the Magellanic Clouds, enabling detailed studies of their star formation history, structure, and stellar populations.
Contribution
It provides the first extensive multi-band near-infrared data set for the Magellanic Clouds, facilitating advanced analysis of their star formation and three-dimensional structure.
Findings
Detailed star formation history map of the Small Magellanic Cloud
High-quality data for variable star analysis
Insights into the proper motion of foreground clusters
Abstract
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.…
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