Stellar Variability in the VVV Survey: An Update
  The Vista Variables in the Via Lactea (VVV) ESO Public Survey consists in a near-infrared time-series survey of the Galactic bulge and inner disk, covering 562 square degrees of the sky, over a total timespan of more than 5 years. In this paper, we provide an updated account of the current status of the survey, especially in the context of stellar variability studies. In this sense, we give a first description of our efforts towards the construction of the VVV Variable Star Catalog (VVV-VSC). 
M. Catelan (1,2), I. Dekany (2,1), M. Hempel (1,2), D. Minniti (1,2)   ((1) Pontificia Universidad Catolica de Chile, (2) Mi...
astro-ph.SR