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: