The path for the PMT calibration data taken by the UCLA setup is as follows:

The DAQ program, known as Automated.vi, runs under LabView on a Macintosh computer. The data is pushed as it is generated, over Appletalk, to a text file on a Linux computer (cos.physics.ucla.edu).

An analysis program, known as PMT, runs on a Sun computer (hepsun5.physics.ucla.edu), which has the disk mounted via NFS. When a batch of phototubes is done, the PMT program can be run. The output of this analysis program is a PAW ntuple in the cos computer area /usr/cdf/pmt/data/.
 

The PAW ntuple is analyzed by hand to make summary plots and decide about phototube acceptance or rejection. A single kumac (plots.kumac) calls other kumacs and fortran routines and outputs to postscript the resulting analysis plots.