Open astrochun opened 5 years ago
mmirs_qrp.main() function with "d-corr" images, which are essentially last - first images determined from the up-the-ramp sampling data. If those "d-corr" files are not available, we need to use the raw data.
Fixes have been implemented: 0a41822d, 7596a13, ee7ac25
Note that an amplifier gain issue is still present to product the true d-corr files.
mmirs_qrp.main() function with "d-corr" images, which are essentially last - first images determined from the up-the-ramp sampling data. If those "d-corr" files are not available, we need to use the raw data.