1st. reduction step:
--------------------
Soon I've reduced all run from 5361 to 5983. The reduced data can be
found in
/brahms/data01/reduced/R5{3,4,5,6}X/seq/
/brahms/data02/reduced/R5{7,8,9}X/seq/
The (relatively few) jobs that crashed or got new Vdrift calibrations will
be re-submitted today.
2nd reduction step:
-------------------
The next step is to find the matching offsets. The db geometry is now
updated (thanks Kris) and I think we found out that magnet problem Djamel
found is not really a problem since the magnetic fields is set again later.
I've put the script I use for the matching in /brahms/data12/match/.
- masterMatch.sh is a simple script that submits bratmain jobs
(PrelReco.C) to CAS. (try option -h).
The matching histograms are saved in /brahms/data12/match/data/ per
default. Using matchOffsets.C and bfsOffsets.C in a root session will
produce the ascii files containing the offsets (ex offset5300_6000.FFS).
I will try to produce standard offsets files (for MRS, FFS, T2_T4, T3_T4
and T4_T5) for all the reduced runs today.
These files are read by BrMatchingOffsetModule (that should be loaded from
brahms_app/do_app/track/libTrackUtil.so).
In parallel we should produce the gtr files (containing global tracks, pid
objects and global info). I suggest we put these in
/brahms/data12/data/gtr/RXXX/seq/. I'll let you know when I've cleaned up
the scripts to do this, they will be put in /brahms/data12/reco/.
3rd redcution step:
-------------------
Making dsts should be relatively simple (and fast). I'll update the
scripts I use for this and put them in /brahms/data12/reco/dst/. ~
Cheers,
Claus
+-------------------------------------------------------------+
| Claus Jørgensen |
| Cand. Scient. Phone : (+45) 33 32 49 49 |
| Cell : (+45) 27 28 49 49 |
| Niels Bohr Institute, Ta-2, Office : (+45) 35 32 53 07 |
| Blegdamsvej 17, DK-2100, E-mail : ekman@nbi.dk |
| University of Copenhagen Home : www.nbi.dk/~ekman/ |
+-------------------------------------------------------------+
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