Hi Dana Why don't you attack version 3.8 available in a few hours. JJ We should submit on friday afternoon. ________________________________ Jens Jørgen Gaardhøje Assoc. prof. Dr. Scient. Chair Ph.D: school of Physics NBI.f.AFG. (secretariat. 35 32 04 41) Chair science committee. UNESCO Natl. Commission. (secretariat. 33 92 52 16) Office: Niels Bohr Institute, Blegdamsvej 17, 2100, Copenhagen, Denmark. Tlf: (+45) 35 32 53 09 Fax: (+45) 35 32 50 16 ________________________________ ----- Original Message ----- From: "Dana Beavis" <Beavis@sgs1.hirg.bnl.gov> To: <brahms-l@bnl.gov> Sent: Tuesday, November 27, 2001 6:19 PM Subject: Re: mult. version 3.6 > HI, > > Two quick comments: > > 1) It might be nice to "fix" a version for a few days so people can comment > on the current version. Then take into account the comments and generate a > new version. The version and comments I have from the weekend may be > obsolete with the new version. > > 2) The title is imprecise. We did not run at the maximum energy. We took > data at the design maximum Au energy. Other species have a different limit > depending on charge to mass ratio. In addition, there has always been talk > of running higher since most of the magnets have a 30% margin. > > **Therefore, I suggest the root(s)=200 GeV to be precise in the title > > > > > >
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