Date: Mon, 23 Apr 2001 15:45:56 +0900 (JST) From: Taku Ishida <ishida@amaterasu.kek.jp> Subject: summary of SciFi meeting Apr.19 2001 Message-ID: <Pine.LNX.3.96.1010423154100.13666A-100000@amaterasu.kek.jp> [Summary of SciFi meeting] KEK TV meeting room 16:00-17:00, Apr.19, 2001 Sakuda/Ishida/Iwashita/Yokoyama/Boyd/Eunju 1) Data analysis - Yoshida's 2001 reprocess is now going. - Iwashita will start Nsk estimation with + MRD1L with ~2000 data. This will reduce systematic error. Check consistency with MRD3D way. - Prepare new data set between "nice" and "cand", which contain all of neutrino interaction candidates in reproc. data. # of events (~2000) fiducial 102,188 Dveto 15,809 -- 1st reduction "nice" goodspill 12,570 Upveto 9,360 <-- ** LG 5,888 spectrum (LG,1L,2D,3D) 4,751 -- 2nd reduction "cand" ** is pure neutrino sample - Addition of new banks (gtrack/kalman/sftntrack) will take place to final samples. Ishida+Steve will discuss final design and commit code this month. 2) MC - Vector generation will be done in the 1st week of May (Hayato). After this FGSIM generation will be started (Yoshida). - Noise parameter for 2001 has been tuned both for CR and for beam by Steve and Yokoyama. They will commit them soon. - After this CR MC will be generated to check CCD-space hit distribution. 3) Improvement of hit finder - 1 dimensional fake hit filter (FC3) is known to be effective to remove parallel ghost tracks. - FC3 will be applied for beam data subset by Steve. - Ishida will continue to develop new fake hit filter with best S/N. 4) CR shift and analysis - We'll continue to take calibration CR data (usually 9:00-13:00 Monday). Shift is assigned. Table is given at Iwashita's desk. - Analysis will be done by Yokoyama ........................................................................ - Sakuda at Kamioka (-Apr.28) - Steve will leave KEK on Apr.28 - Eunju will present K2K results at KPS (Apr.26-May 3rd) ........................................................................ - Next Meeting (TV, May 1st ?) (fin)
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