Ulisse Munari gave a more complete description of their spectrograph CCD readout scheme. If I understand it properly, then I understand why they use such a long read time. Like I said earlier, as you shorten the read time, you increase the readnoise. However, as you lengthen the read time, you will eventually come to the point where you start losing correlation between the two correlated-double-sample reads, and readnoise again increases (or at least reaches an asymptotic limit). I think the main reason for Munari's long read time is contained in the statement: >...to achieve the >100 m/sec EXTERNAL precision in the radial velocities of suitable >cool stellar targets, charge transfer wake effects must be taken >under strict control (particoularly with the strong lines in the >comparison spectrum). I have seen clear degradation in the >radial velocity accuracy with faster read-outs. That is, the longer read time permits proper waveform shaping and control of CTE effects; this is not the same as getting minimum read noise. I fully agree and support his other comments regarding filtered observations rather than unfiltered ones! Arne