User name van Westrum
Log entry time 02:31:04 on November 2,1997
Entry number 573
keyword=SOS Gas cerenkov spectra!Finally, we get to see these argonne mirrors in action. these are the first, most raw, spectra (I haven't had a chance to set thresholds, or scheck efficiencies). Will do that tomorrow, but without further ado,
note that the scer versus x doesn't have that crappy sag-factor anymore. more later.
FIGURE 1
