Post CARA Plans
Map CMB with 4 beam (ACBAR)
Study high order acoustic peaks in CI spectrum
Determine unequivocally whether galaxy cluster
contain non-baryonic dark matter through SZE
studies of low z clusters.
Survey galaxy clusters at high redshift through SZE
Measure cluster peculiar velocities
Guest Observations
Extend sub-mm uses of Viper
SPARO
Larger arrays
Test bed for arrays built for ten meter.
Guest Observations
CMB polarization at high frequencies