4MOST is the next generation wide-field
spectrograph for surveys at ESO. The five year
survey will yield more than 10 million medium
resolution spectra of stars across all stellar
populations in the Southern Hemisphere as well as
more than 3 million high-resolution spectra for
stars in the disk and Galactic bulge. Learn more
about 4MOST by reading our webpages. If you are
interested to join please contact us.
WEAVE is an instrument, a survey, and a
collaboartion which will provide more than 4 million
stellar spectra in the Northern Hemisphere.
This is a large European collaboration lead by Gerry
Gilmore and Sofia Randich. The survey is about to
complete in 2018 and has carried out 300 nights of
in visitor mode with the FLAMES spectrograph on
VLT. You find all Gaia-ESO publications on
SAGA is a photometric survey using the Strömgren
filter system. The observations have been carried
out with the prime focus Wide Field Camera at the
INT on La Palma.