The collaboration has used a 518 k Ci Cr neutrino source to test the experimental operation. The energy of these neutrinos is similar to the solar Be neutrinos and thus makes an ideal check on the experimental procedure. The extractions for the Cr experiment took place between January and May 1995 and the counting of the samples lasted until fall. The result, expressed in terms of a ratio of the measured production rate to the expected production rate, is 1.0 ± 0.15. This indicates that the discrepancy between the solar model predictions and the SAGE flux measurement cannot be an experimental artifact. Also calibrations with a Ar neutrino source had been performed.