Thursday 21st April 14:00 BST; we will be in the MICE meeting room in R1.

Phone details:


Rogers and Victoria:
  • "Top-down" list of plots
  • The low-level track reconstruction (everything up to pattern recognition) should be written up ASAP. I think it is at a reasonable point?
Chris Hunt: Scott and Tanaz:
  • What is the impurity reported by MC, based on Scott cuts?
  • Can we confirm that the muon shoulder arises due to diffuser? i.e. extrapolate reconstructed tracks back to the diffuser position, what is the radius?
  • Any results for likelihood-based PID?
Jan and Rogers:
  • What is the source of disagreement between TOF and tracker?
    • What is the material budget between TOF and tracker? Is it correct?
Joe and Victoria:
  • Are the OPERA model and Hall probes consistent? How big are the
  • Continue trying to untangle the field mapping data for SSU
  • Why do we not see the muon shoulder in MC? Is the material done right in the fringes? Diffuser, Shoulder, Shoulder_MC
  • Are there any other discrepancies? Plots
  • Can the agreement between MC and data be improved?
    • At what statistical significance do MC and data disagree?
    • What are the systematic errors (e.g. from quad/dipole/solenoid settings, incorrect material model etc)?
  • Emittance calculation etc - any updates?

diffuser_mat.png (9.87 KB) Drielsma, François, 21 April 2016 12:46

pz_tof01.png (26.5 KB) Drielsma, François, 21 April 2016 12:46

pz_tof01_mc.png (27.2 KB) Drielsma, François, 21 April 2016 12:46 (1.25 MB) Drielsma, François, 21 April 2016 12:48

PID_TanazA.Mohayai.pdf (1.21 MB) Mohayai, Tanaz Angelina, 21 April 2016 14:01

p-p_pid.pdf (37.5 KB) Wilbur, Scott, 21 April 2016 14:51