C.10 From Revolution 103

1. Reset intervals of 4 seconds allowed for band 1 detectors. This occasionally gives better sensitivity.
2. Further change to longer dark-current measurements. This gives better baselines for some cases.
3. Reference scans bracketing short scans suppressed in SWS06. This gives higher observing efficiency for some cases.
4. FP minimum scan repetition changed from 2 to 3-fold giving more redundancy.
5. Wavelength-dependent FP gap correction giving improved tracking between FP and grating, especially at shorter wavelengths. Worth mentioning