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Hi Lamiaa,<br>
<br>
Tcl and list of files look fine.<br>
Please proceed with cooking of 6 GeV data.<br>
<br>
Thanks, Stepn<br>
<br>
On 2/15/11 10:02 PM, Lamiaa El Fassi wrote:
<blockquote
cite="mid:AANLkTikB70xLUkJZk8rggoSx+bzfv5XCeXAfGg0sdxCB@mail.gmail.com"
type="cite">Hi Stepan,<br>
<br>
As it was mentioned this morning on our weekly meeting, I will
process the full 6 GeV data set <br>
with the IC calibration constants that we have right now in our
database and without any CC time <br>
calibration constants. <br>
<br>
As a reference, I am attaching a list of the 6 GeV good production
runs and also the tcl file that <br>
I am willing to use. It's similar to the 5.7 GeV tcl file.<br>
<br>
The 6 GeV cooking strategy is: <br>
<br>
1. Produce the regular outputs: <br>
a. SEB ntuple<br>
b. H2ROOT & CLASTOOL Root ntuples<br>
c. BOS file<br>
d. ANAHIST file<br>
e. Helicity correction text file<br>
f. LOG file<br>
<br>
2. Saved all outputs on SILO under a branch:
/mss/clas/eg6/production/pass1_v0/6gev/<br>
<br>
3. Since we are still using 2.8 TB disk space of our private work
disk for 1.2 GeV outputs, <br>
I will save only the outputs (d & e) on our disk, however,
the other formats will be linked <br>
to their own branches under a main directory:
/work/clas/claseg6/top_dir/pass1_v0/6gev/.<br>
Of course, all links are accessible until they get deleted
from the auto-managed work disks. <br>
<br>
Please feel free to send me any suggestions or requests by
tomorrow afternoon.<br>
<br>
Best regards,<br>
<br>
Lamiaa<br>
<br clear="all">
************************************************************<br>
* Lamiaa El Fassi email: <a moz-do-not-send="true"
href="mailto:lamiaa11@fnal.gov">lamiaa11@fnal.gov</a><br>
* Research Associate @ Rutgers University <br>
* Phone: (630) 840-4861 <br>
* Fermilab, Aspen East #105 <br>
* Batavia, IL. 60510<br>
************************************************************<br>
<br>
</blockquote>
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