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UPDATES TO BE DONE: 1. Links broken
Current estimates are that the overheads associated with each new science target (for target acquisition, telescope, WFS and instrument re-configuration etc) depend upon the guide configuration chosen for the observation.
Setup times for various observation types are:
This section contains information on the sensitivity and performance of NIFS in its various observing modes. Go directly to:
All links will need updating when GNIRS pages are in place
The optical elements of GNIRS (e.g. cameras, gratings, cross-dispersing prisms and slits) are described in detail on the GNIRS components (broke) pages.