Hello, Nick 1. I think there is no generic approach for arbitrary Zebra-bank. 2. STAR does convert GEANT3 track / hits / geometry to STAR C++ OO based on TDataSet / TTable / TVolume model "on fly". 3. No ZEBRA "DST" experience though. Let me know whether it is insteresting enough and you want further information. Best regards, Valeri ----- Original Message ----- From: "Nick van Eijndhoven" <Nick@phys.uu.nl> To: "ROOT discussion group" <roottalk@pcroot.cern.ch> Sent: Wednesday, May 23, 2001 11:23 AM Subject: [ROOT] ZEBRA->ROOT > Dear friends, > I have some DST files containing experimental physics data in ZEBRA format. > To analyse the stuff I would like to use ROOT. To my opinion the best > procedure for this is to convert the ZEBRA files into ROOT trees. > I know how to do this for ntuples, histograms etc... (i.e. h2root) > but have no idea how to tackle this for plain ZEBRA banks. > Could one of you tell me the most efficient way to get this done. > > Thanks in advance, > Nick. > -- > Dr. Nick van Eijndhoven mailto:nick@phys.uu.nl http://www.phys.uu.nl/~nick > -------------------------------------------------------------------------- > Org.: Utrecht University/Nikhef, Department of Subatomic Physics > Address: P.O. Box 80.000, NL-3508 TA Utrecht, The Netherlands > Phone: +31-30-2532331(direct) +31-30-2531492(secr.) Fax: +31-30-2518689 > NIKHEF: +31-20-5922178(direct) +31-20-5922000(secr.) Fax: +31-20-5925155 > CERN: +41-22-7679751(direct) +41-22-7675857(secr.) Fax: +41-22-7679480 > Offices: Buys Ballot lab. 710 (Utrecht) N241 (Nikhef) B23 1-020 (CERN) > -------------------------------------------------------------------------- >
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