Some Proposed Surveys
Next Decade: New optimized ėsurvey systemsî
exploring new parameter space
Dark Matter Telescope
map the distribution of matter for z<1.5 from weak lensing, through deep, high quality images of galaxies
moving and variable objects through repetitive surveys
Spectroscopic Wide-Field Telescope
evolution of galaxies from z~4 to the present from star formation rates
determine chemical abundances and kinematics
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