Catalin, I guess this really doesn't mean much for most people, but there is nothing different in the dsts for the flow data for run04 auau 200. I needed to make a change to how the data was processed in order to properly process the run05 flow data. Erik ________________________________ From: brahms-dev-l-bounces_at_lists.bnl.gov on behalf of Catalin Ristea Sent: Sun 7/9/2006 3:38 AM To: brahms-dev-l_at_lists.bnl.gov Subject: [Brahms-dev-l] dst rerun for auau_at_200, run04 Hi, Yesterday the rerun for a new dst version was completed. Current production version is 3. Changes from the previous versions: - got in the global chi2 for the mrs tracks. - updates to the flow modules. I'll start looking over the mrs data. Kind regards, Catalin. -- Catalin Ristea--------------------------------- High Energy and Heavy Ions Group Niels Bohr Institute Blegdamsvej 17, 2100 Copenhagen, Denmark Tel (+45) 35 32 54 04 / Fax (+45) 35 32 50 16 E-mail: catalin.ristea_at_nbi.dk http : www.nbi.dk/~ristea ----------------------------------------------- _______________________________________________ Brahms-dev-l mailing list Brahms-dev-l_at_lists.bnl.gov http://lists.bnl.gov/mailman/listinfo/brahms-dev-l _______________________________________________ Brahms-dev-l mailing list Brahms-dev-l_at_lists.bnl.gov http://lists.bnl.gov/mailman/listinfo/brahms-dev-lReceived on Sun Jul 09 2006 - 11:54:51 EDT
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