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The main aim of this experiment is to provide a complete census of old (t >10 Gyr, RR Lyrae, type II Cepheids, red horizontal branch), intermediate age(red clump, Miras) and young (classical Cepheids) stellar tracers across theGalactic Bulge. To fully exploit the unique photometric quality of LSST images,we plan to perform a Shallow minisurvey (ugrizy, -20 < l < 20 deg, -15 < b < 10deg) and a Deep minisurvey (izy, -20 < l < 20 deg, -3 < b < 3 deg). The formerone is aimed at constraining the 3D structure of the galactic Bulge across thefour quadrants, and in particular, the transition between inner and outerBulge. The u,g,r,i,z,y LSST bands provide fundamental diagnostics to constrainthe evolutionary properties of low and intermediate-mass stars when moving froma metal-poor to a metal-rich regime. The deep minisurvey is aimed at tracing RRLyrae, Red Clump stars, Miras and classical Cepheids in highly reddened regionsof the Galactic center. These images will allow us to investigate the role thatbaryonic mass and dark matter played in the early formation and evolution ofthe MW.

unVEil the darknesS of The gAlactic buLgE (VESTALE)