NAME¶
pyFAI-average - pyFAI-average
DESCRIPTION¶
usage: usage: pyFAI-average [options] [options]
-o output.edf file1.edf
file2.edf ...
This tool can be used to average out a set of dark current images using mean or
median filter (along the image stack). One can also reject outliers be
specifying a cutoff (remove cosmic rays / zingers from dark)
positional arguments:¶
- FILE
- Files to be processed
optional arguments:¶
- -h, --help
- show this help message and exit
- -V, --version
- show program's version number and exit
- -o OUTPUT, --output OUTPUT
- Output/ destination of average image
- -m METHOD, --method METHOD
- Method used for averaging, can be 'mean'(default) or 'median', 'min' or
'max'
- -c CUTOFF, --cutoff CUTOFF
- Take the mean of the average +/- cutoff * std_dev.
- -F FORMAT, --format FORMAT
- Output file/image format (by default EDF)
- -d DARK, --dark DARK
- Dark noise to be subtracted
- -f FLAT, --flat FLAT
- Flat field correction
- -v, --verbose
- switch to verbose/debug mode
It can also be used to merge many images from the same sample when using a small
beam and reduce the spotty-ness of Debye-Sherrer rings. In this case the
"max-filter" is usually recommended.