Known issues with the instrument and telescope are:

  • Unexpectedly low efficiency in u and U.
  • Unexpectedly high dark current in C0 (the ugri and UBV camera).
  • Optical mode (guiding with one of the science CCDs) has not been fully characterised.
  • C2/C3 are currently not available, but C4 is serving in their place.
Last modified 2 years ago Last modified on May 21, 2015 3:36:42 AM