From 2009 on the MCSF was periodically imaging the entire Large and Small Magellanic Cloud using the RoBoTT (formerly Vysos 6) robotic telescope at the Universitätssternwarte Bochum in Chile. From June 2009 to January 2010 the SMC has been observed monthly in B,R and Hα (+ S[II], O[III] and V in one month) giving us a robust temporal resolution on intermediate timescales. Additionally the SMC has been visited in July and August 2011 to take two full sets of observations in u, B, R, V, I and Hα, O[III], S[II]. The LMC has been surveyed once a year (B,R, Hα in 2009 and 2010; u, B, V, R, I and Hα, O[III], S[II])

The 2009 and 2010 observations include short exposure frame of 10 to 40 seconds (depending on the filter) to ensure that the brightest stars stay unsaturated.

This unique dataset gives us the oppertunity to study the stellar populations up to ~ -10 mag as well as the stellar feedback from the most massive stars.

The data will successifely be made public available. Currently we can give no exact roadmap for the data releases. However, you have a first look at the images in our image gallery. A first insight in our photometric data is given by presenting Color-Magnitude-Diagrams of the Magellanic Clouds under "Results".

For early data access please contact: abecker@astro.rub.de.