Mapping the milky way in the near-IR: The future of the VVV survey

Research output: Chapter in Book/Report/Conference proceedingChapterpeer-review

23 Citations (Scopus)


The VISTA Variables in the Via Lactea (VVV) is an ESO public survey that has been mapping the bulge and inner disk of the Milky Way in the near infrared for the past 6 years. Here we examine the scientific goals and some key results, as well as the legacy of the VVV survey. We also discuss the making of the first huge public image of the Galactic bulge (a 140 Gigabytes single image with 25,000 Megapixels), and how these data allowed us to measure directly the total bulge mass of the Milky Way bulge, that is twenty billion Solar masses. Finally, we present the plans of the recently approved VVVX, an extended survey of the Milky Way, that would map about 4% of the sky repeatedly in the near-IR, measuring more than 2 billion stars, producing a ~1 Petabyte database (containing images, catalogues and maps) for the whole community to exploit.

Original languageEnglish
Title of host publicationAstrophysics and Space Science Proceedings
PublisherSpringer Netherlands
Number of pages9
Publication statusPublished - 1 Jan 2018

Publication series

NameAstrophysics and Space Science Proceedings
ISSN (Print)1570-6591
ISSN (Electronic)1570-6605

ASJC Scopus subject areas

  • Physics and Astronomy(all)
  • Computer Science Applications
  • Spectroscopy
  • Space and Planetary Science
  • Nuclear and High Energy Physics


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