- Gemini Home
- Telescopes and Sites
- Science Visitors at Gemini
- Observing With Gemini
- Retired Instruments
- Visiting Instrument Policy
- Visiting Instrument Telescope Interfaces
- DSSI Speckle Camera
- TEXES (North)
- Integration Time Calculators
- Magnitudes and Fluxes
- Near-IR Resources
- Mid-IR Resources
- Observing Condition Constraints
- Performance Monitoring
- SV/Demo Science
- Future Instrumentation & Current Development
- Queue and Schedules
- Data and Results
- Gemini Research Staff
Change page style:
Natural Seeing (Non-Adaptive Optics) Guided Observations:
NIRI standalone (i.e., without AO) requires the use of a peripheral wavefront sensor for both imaging and spectroscopy. PWFS2 is preferred over PWFS1, as it can be used on fainter guide stars, can run at a higher frequency for a given guide star, works better under windy and cloudy conditions, and is smaller and thus vignettes less of the field of view.
f/6 imaging: PWFS2 guide star should be located >5' from the target
f/14 and f/32 imaging and spectroscopy: PWFS2 guide star should be located < 4.25' from the target. For guide stars closer than 5' the position editor in the Observing Tool should be inspected carefully to check that the PWFS probe does not block the science field. The outer limit for PWFS2 guide stars can be displayed on the OT position editor.
Laser Guide Star (LGS) and Natural Guide Star (NGS) Adaptive Optics (AO) Guided Observations:
In NGS and LGS mode, NIRI is paired with the ALTAIR natural/laser guide star adaptive optics system.
NGS: The guide star (which may be the target itself) is used to provide wavefront information for the deformable mirror as well as overall image motion for tip/tilt
LGS: The laser created guide star provides information for the deformable mirror while a nearby star must be used for tip/tilt. This star can be much fainter than an NGS star used with the deformable mirror.