Known problems and limitations

• Times within Kvis are treated as UT hours with no date information. This means that multi-day data files (which do not normally occur) and files which contain the 24 UT to 0 UT transition are not handled properly (note: this boundary is during the day in Hawaii and so will not occur in standard night observing).

• All possible bad values of parameters in ini.params and config.params are not checked for.

• The numbers of spectrometer channels and wavelengths must be constant throughout the archive files (or the specified start and stop times if given). The fringe tracker rate may change.