Capability Summary
- Extreme adaptive-optics (AO)
- Contrast ratios of 106 (at separations of 0.2–1", in 1-hour)
- Total wavelength range = 0.9−2.4 µm
Plane options
- Coronagraphy (APLC)
- Direct (no APLC)
- Non Redundant Mask (NRM)
Modes
- Spectroscopy (Read more)
- IFU (R ≈ 40)
- 2.4" square field of view
- 0.014" per lenslet spatial sampling
- YJHK spectral ranges (K band is split)
- Polarimetry (Read more)
- Dual channel polarimeter (full field)
- bands (Y, J, H, K1 or K2).
GPI has been built by a consortium of U.S. and Canadian institutions, funded by the Gemini Observatory, which is an international partnership comprising the U.S.A., U.K., Canada, Australia, Argentina, Brazil & Chile. The GPIES campaign is partially funded by NSF, NASA, the University of California and the Laboratory Directed Research and Development funding at the Lawrence LIvermore National Laboratory.
Announcements
Instrument Team
Instrument Scientist
