The official sample was produced by David Saltzberg (electrons) and Mark Krasberg (muons) from Stream 2 DST (?) tapes.
We stripped through all (131) Stream A DST tapes. We take all volunteeers, i.e. there is no requirement on the trigger path
Note that all values are taken straight from the ELES banks that we got from production. For example, momenta are NOT beam-constrained.
Again, all values are taken straight from the CMUO banks that we got from production. No beam constraining is done.
PAD format, see c$examples:pad_banks.uic
The electron data set is sitting on UCCDFL$DKA400 and UCCDFQ$DKA100. Use C$ALLDAT:ICE_CC*.PAD to get it. Muons are on UCCDFP$DKA100. To get them use C$ALLDAT:WZ_CM_CC*.STRX_3P*
The data sets sit on disks on UCCDFM, UCCDFP and UCCDFQ. The easiest way to get them is to use `c$alldat:ICEFLT*.STRX_PAD*' for electrons and `c$alldat:CMUFLT*.STRX_PAD*' for muons. Make sure you use the astrisk at the end as there are various file extensions (like *.strx_pad_plus or *.strx_nodup). You should get 131 files each for electrons and muons. If you don't, there is a problem !