CARMA Spectral Line Correlator Requirements 
M. C. H. Wright 
Radio Astronomy Laboratory, 
University of California, Berkeley, CA, 94720

We review the expected sensitivity and spatial dynamic range of the
CARMA array during the next 10 years in comparison with the ALMA,
ACA, SMA and IRAM arrays. The scienti£c capabilities of the CARMA
array can be greatly enhanced at modest cost by adding a full
polarization spectral line correlator.