SCORPIO is our next facility-class instrument, designed for follow-up studies of transients in the Rubin Observatory era while carrying out with high efficiency a large variety of astrophysical programs. SCORPIO will be a
A contract to design, build, and commission the instrument was signed between the Southwest Research Institute (SwRI) in San Antonio, Texas, and the Association of Universities for Research in Astronomy (AURA) in March 2017. The project completed the Critical Design Stage in 2020 and the project is now progressing through the build phase. Commissioning is expected for early 2024.
Gemini has contracted with the Australian Astronomical Observatory (AAO) for the continued design and construction o
GHOST will provide two-object plus sky spectroscopy with full wavelength coverage from ~363 - 950
IGRINS-2 will be a high-resolution near-infrared spectrograph (R ~ 45,000; 1.45 - 2.50 μm), closely based on the original IGRINS (Immersion GRating INfrared Spectrograph). Unlike IGRINS, being used as a visiting instrument at Gemini South, IGRINS-2 will be a full facility instrument when it comes to Gemini North.
After successfully completing design reviews, the IGRINS-2 project is currently in the build phase led by the Korea Astronomy and Space Science Institute (KASI) in Daejeon, Korea. We are aiming for commissioning of IGRINS-2 in late 2023 and offering it to the Gemini science community in late 2024.
The GIRMOS project is led by the University of Toronto (UofT) Dunlap’s Prof. Suresh Sivanandam, and is being funded through a Canadian Foundation for Innovation award plus contributions from other partners. GIRMOS is intended to provide Gemini with high performance adaptive optics multi-object integral field spectroscopy, with a parallel imaging capability, and will take advantage of the future Gemini North Adaptive Optics facility (GNAO). GIRMOS will be able to observe four objects simultaneously within the GNAO field-of-regard or a single object by tiling the four integral field units. Working in parallel with the spectrographs, GIRMOS’s imager will reach the telescope the diffraction limit in H-band over a 85′′×85′′ imaging field, with just minor vignetting from the spectroscopic pickoffs when they are deployed. Gemini is presently funding the preliminary design study of the GIRMOS imager subsystem, providing in-kind staffing in overall project systems engineering, and other aspects of the project.