  We use arcminute-scale data from the Sunyaev-Zel'dovich Infrared Experiment
to set limits on anisotropies in the cosmic microwave background radiation in
open and spatially-flat-Lambda cold dark matter cosmogonies. There are no
2-sigma detections for the models tested. The upper limits obtained are
consistent with the amplitude of anisotropy detected by the COBE/DMR
experiment.
