<div>Hi FX,</div>
<div> </div>
<div>Yes, the root and BOS files were copied to the auto-managed work disks </div>
<div>and the SEB ntuple and ANAHIST files were saved on the claseg6 work </div>
<div>disk. Since they get deleted the fastest way to reproduce at least the HROOT </div>
<div>files is to run the "h2root" over the SEB ntuples. </div>
<div> </div>
<div>Please let know if you experience any difficulties so I can recook again a bunch </div>
<div>of files, and, sorry for any inconvenience!</div>
<div> </div>
<div>Best,</div>
<div> </div>
<div>Lamiaa </div>
<div> </div>
<div>************************************************************<br>* Lamiaa El Fassi email: <a href="mailto:elfassi@jlab.org">elfassi@jlab.org</a><br>* Research Associate @ Rutgers University <br>
* Phone: (757) 269-7011 // Fax: (757) 269-5703 <br>* Jefferson Lab., 12000 Jefferson Ave. <br>* Suite# 4, MS 12H3<br>* Newport News, VA. 23606<br>************************************************************<br>
<br><br></div>
<div class="gmail_quote">On Tue, Jun 29, 2010 at 4:40 PM, <<a href="mailto:fxgirod@jlab.org">fxgirod@jlab.org</a>> wrote:<br>
<blockquote class="gmail_quote"><br>Dear Lamiaa,<br>
<div class="im"><br>> As a reminder of the 64 bit jobs that I have processed earlier, could any<br>> one volunteer to do the event-by-event check, as Stepan suggested, with<br>> the<br>> same 32 bit files? I didn't notice any difference between the saved tracks<br>
> or particles numbers saved on the CSQL database, however, a detailed<br>> comparison is needed. It is important to converge on that soon to start<br>> using the 64 bit farm nodes.<br><br></div>I wanted to try this check, but I cannot seem to find the 64 root ntuple<br>
format.<br>Have they been copied only to the work discs ?<br>If so, which is the fastest way to re-produce them ? Can I just run h2root<br>on one of the other directory ?<br><br>Thank you for your help,<br>Best regards,<br>
FX<br><br></blockquote></div><br>