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Updates in SNOMAN 4.02

The major changes in version 4.02 include the addition of many more fields in the FTM output bank.

Several values are filched from the monte-carlo if the MC banks are present when FTM is run. This allows such items as the stopping position of the muon to be compared to the fit.

The impact parameter of the muon is found to be highly subject to fitter pull. An analytic expression is used to move the impact parameter from $P_fit$ to $P_corrected$, which is corrected systematically for fitter pull. This is stored in the KFTM_pcorr word. Note that this correction is a function only of $P_fit$, not of any other parameter, and is based on MC assessments of the muon fitter.

The most important change in version 4.02 is the inclusion of an assortment of goodness-of-fit parameters that can be used to determine if the fit hypothesis is good. It is NOT recommended that the chi-squared parameter be used for this.

Two values in particular are important:

KFTM_FShould: This parameter indicates the fraction of tubes in the track forward Cherenkov cone that fired. That is, a value of 0.95 means that 95% of all the tubes that SHOULD have fired due to direct Cherenkov light did in fact fire. Good fits should have an FShould parameter of greater than 0.8. Bad fits will have values less than 0.5.

KFTM_pdf_dof: This parameter is a summed log-likehoold of time residuals for all the tubes in the event, dividied by the number of tubes. The pdf function used to create the log-likelihood is a piecewise continuous function created using the time residuals from MC muons. Larger values of the parameter indicate worse fits. Good fits typically have pdf_dof values less than 4.5. Exteremely bad fits will have values of about 6.5.

For more information on the operation of the Muon Fitter, refer to Nathaniel Tagg's Ph.D. thesis.


next up previous contents
Next: Path Fitter Up: Muon Fitter Previous: Updates in SNOMAN 3.02   Contents
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