Residuals, cosmic run 40-45 with Gaussian fits
Residuals with gaussian fits over strips.
To make sure that one actually fit a gaussian I extended 1 and 2 strip wide clusters to 3 strips
The difference to the charge weighted residuals is neglible
First, fit chi2/ndf and fit status (0==good)
Disk2, x direction:
Disk 1:
Disk3:
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