Message-Id: <200103030958.SAA17337@neutrino.kek.jp> Subject: Re: Minutes of SciFi weekly meeting (01/Feb/28) Date: Sat, 03 Mar 2001 18:58:01 +0900 From: Makoto Sakuda <sakuda@neutrino.kek.jp> > To: sakuda@neutrino.kek.jp > Cc: hasegawa@neutrino.kek.jp, e362scifi@neutrino.kek.jp, lbkek@neutrino.kek.jp > Subject: Re: Minutes of SciFi weekly meeting (01/Feb/28) > From: Yoshinari.Hayato@kek.jp > In-Reply-To: <200103030614.PAA29404@neutrino.kek.jp> > References: <200103030614.PAA29404@neutrino.kek.jp> > > Dear Sakuda-sensei, > > I think it is better to prepare the description of the > analysis (what kind of the events are used to estimate the > background and what kind of the events are used to estimate > the flux) and the efficiencies at each event selection > criteria, you have applied. > At the same time, we may want to know the purity (S/N) and > background(misidentified particles) of the candidate tracks, > for both muon and proton. > > These informations are also quite important for the > evaluation of our Monte-Carlo, especially the purity and > contamination of the primary and secondary tracks. > > Best regards, > Yoshinari Hayato > Hello, We are finishing the official plots based on the previous K2K talks. I think that the official area should make the analysis clearer and answer most of your questions. Please discuss with Chris and Steve about the flux analysis and the Web page. Explanation of samples is there. Selection criteria -- one page (in ps file) will be added. We will discuss more on official plots at the weekly meeting. MC related figures that you requested for Friday NEUT meeting will be discussed at the meeting too. Agenda 1. Official plots 2. Goals for June 24/25 meeting Regards, M.Sakuda
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