Vista variables in the via lactea (VVV): First results and perspectives

R. K. Saito, D. Minniti, I. Dékány, M. Hempel, J. Alonso-García, I. Toledo, J. C. Beamin, R. Angeloni, P. W. Lucas, J. P. Emerson

Research output: Contribution to journalArticlepeer-review

6 Citations (SciVal)


VISTA Variables in the Vía Láctea (VVV) is a public ESO near-IR variability survey scanning the Milky Way Bulge and an adjacent section of the mid-plane. The survey will take 1929 hours of observations with the 4 m VISTA telescope during five years (2010-2014), covering ∼ 109 point sources across an area of 520 deg2. Here we address the first results obtained from the VVV Survey as well as a glimpse into the possibilities for using a deep near-IR atlas in five passbands and a catalogue of more than 106 variable point sources. We expect to use the data to find planetary transits of late-type main-sequence stars. We discuss the planet searches and future follow-ups.

Original languageEnglish
Pages (from-to)221-224
Number of pages4
JournalRevista Mexicana de Astronomia y Astrofisica: Serie de Conferencias
Publication statusPublished - 2011


  • Galaxy: Bulge
  • Galaxy: Disk
  • Planets and satellites: General
  • Stars: Variables: General
  • Surveys

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics


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