VISTA Variables in the Vía Láctea (VVV): Current Status and First Results
VISTA Variables in the Vía Láctea (VVV) is a public ESO near-IR variability survey aimed at scanning the Milky Way Bulge and an adjacent section of the mid-plane. VVV observations started in October 2009 during ESO science verification. Regular observations for the first year of the survey have been conducted since February 2010 and will cover a
Saito, R. et al.
Fecha de publicación:
9
2010