February 17, 2009 Physics

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Calibration

  • Reconstructed Z minus generated Z over the length of the module. The deviations are less than 0.5 cm.

MeanrecZ minus genZ.png


  • Reconstructed single photon (0 to 4 GeV) energy BEFORE corrections

A flat correction has been made for sampling fraction and smearing has been applied in DBCALMCResponse. The threshold is a flat 6 MeV/segment.

RecEgenE vs recZ.png RecEgenE vs recZ mean.png


  • Fit function for reconstructed energy for slices of z along the BCAL
{\frac  {E_{{rec}}}{E_{{gen}}}}=A*E_{{gen}}^{{\alpha }}+B/E_{{gen}}

so that

E_{{gen}}=({\frac  {E_{{rec}}-B}{A}})^{{{\frac  {1}{1+\alpha }}}}

H31 1 sum nCellLT5.png


  • Fit function for parameter A, \alpha, and B


A=par0*(1+par1*exp({\frac  {1}{2}}{\frac  {(Z-par2)^{{2}}}{par3^{{2}}}}))
\alpha =par0+par1*exp({\frac  {1}{2}}{\frac  {(Z-par2)^{{2}}}{par3^{{2}}}})
B=par0+par1*exp({\frac  {1}{2}}{\frac  {(Z-par2)^{{2}}}{par3^{{2}}}})

"A" "\alpha" "B"



Reconstruction

  • Reconstructed single photon (0 to 4 GeV) energy AFTER corrections

EPhogenE vs recZ.png EPhogenE vs recZ mean.png


Figure512.png


Figure513.png

Semi-parametric Monte Carlo

Here are some slides David showed at this meeting.


Thoughts, to do list, etc. from meeting

Z.P., B.L., D.L., M.S., R.M.

1. look at difference between reconstructed and generated z position for less than 65 cm
2. look at single photon reconstruction efficiencies
3. adjust the error matrix for the BCAL (look in PID/DPhoton_factory.cc)
Next Steps:
1. look at the a2 mass peak - adjust cuts on the eta and pi0 masses
2. introduce Pythia background - skim off the wanted events by cutting on the total neutral energy (but we need to record the total number of events before skimming) - hd_filter is a good program example
3. cut on eta and pi0 masses, then look at the effect on the different angular distributions (i.e. Gottfried-Jackson angles, etc.)