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Hi all, this is a breif update on the neutral and D*0 state. On the D*0 side: a) Run-1 seems validated. you can see http://www.slac.stanford.edu/~asarti/garbage/prova4 and compare with http://www.slac.stanford.edu/~asarti/garbage/prova4 (# of events is slightly different because of a job has crashed: this will be fixed soon) Number of events, and purity will come soon (problem with the argus fit on root). b) Run-2 production has already started on Lyon ! On the neutrals side: Mnu2 plots are starting to look better (means like what was shown by Daniele: http://www.slac.stanford.edu/~asarti/recoil/21112001/Mnu_root.ps ). The prevoius discrepancies were due to missing cuts on the purity of the B in the events and the missing requiremnt of correlation on event charges..) We have studied gammas: Energy, phi and theta. Phi seems to be not promising (flat distributions..) Theta and E are objcet of a deeper study (as preliminary result on theta you can see http://www.slac.stanford.edu/recoil/19112001/ratio_theta_gam.eps) We are planning to look at the combination of Energy and Theta... We want to optimize the resolution of Mx and the quantity: r = #vub / sqrt( #vub + #vcb) But we are waiting for the sideband subtraction.. comments and questions are welcomed, Alessio ______________________________________________________ Alessio Sarti Universita' & I.N.F.N. Ferrara tel +39-532-781928 Ferrara "Che il bianco sia bianco, e che il nero sia nero che uno e uno fanno due e che la scienza dice il vero.... DIPENDE !" On Mon, 19 Nov 2001, Urs Langenegger wrote: > > Hoi, > > there is quite a bit we need to get done for the collaboration > meeting. The following is a list of the things we considered most > important. We'd like to discuss this list in a *short* meeting on > > Wednesday, 11/21/01, 8:30 am PST, at SLAC: Pom/Flora > Call 1-510-647-3480, press 1, enter 171023# > > It would be good especially to learn about the status and prospects of > items marked with '=>' below. > > > Cheers, > > Daniele & > --U. > > > ---------------------------------------------------------------------- > Data Production > --------------- > -> Validation of Run 1 Dstar0 -> Alessio > Run 1 D0 -> Daniele > -> Convert to Kanga Files (Run1 B+) -> Urs > -> Run 2 (prewinter dataset) > -> generate TCL files -> Daniele > -> run jobs -> Daniele, Alessio, Oliver, Giancarlo > -> generate tables -> Daniele > -> Convert to Kanga Files (Run2) -> Urs > > > Ntuple Production > ----------------- > -> Beta code modifications > -> likelihood e/mu selector -> Daniele > -> mod pi0 list name -> Daniele > -> add conversions -> Ric (as it turned out) > > -> Rerun production with -> Urs > Dstar, Dc, Dstar0, D0 > > > Analysis > -------- > -> Data/MC comparison for variables -> Oliver/Urs/Daniele > mes, deltaE, > Mx, > mm2, neutrino direction, |pmiss| > q2 > p*, cosTheta, charge correlation to BRECO > sum(q_i), multiplicities > .... > -> Crossfeed studies -> Urs > -> Wrap kin fitting into root analysis -> Oliver/Urs > -> Fit: convert to root -> Daniele > > => Neutrals: Emin? pi0? other algorithms? -> Alessio > => KLongs: What will be avaiable on what timescale? -> Giancarlo, Guglielmo >