Probing Galactic Structure With Musyc

We present some preliminary results of the Galactic program within the MUSYC collaboration. Using the multi-colour photometry of MUSYC we are able to classify objects and select samples of a given type. We apply colour selection to establish a sample of M-stars in the MUSYC field CDFS-E which was then used to study the distribution along the pencil beam. The distribution shows three components for which we derived scale heights indicating that these components are the Thin and Thick Disk and the Halo.http://www.redalyc.org/articulo.oa?id=57102627