We present a status update on SCORPIO, the next facility instrument for the Gemini South telescope at Cerro Pachon, Chile. SCORPIO is now in advanced Assembly, Integration and Verification phase at SWRI (San Antonio) and LICA (Madrid) in anticipation of shipment to Chile by Fall-2025.
SCORPIO (Spectrograph and Camera for the Observation of Rapid Phenomena in the Infrared and Optical) is a multiband instrument covering 0.385um to 2.35um in spectroscopy and 0.400um to 2.35um in imaging, currently under development for the Gemini Observatory. The instrument is intended to be deployed as a facility instrument at Gemini South in Chile to enable detailed follow-up observations of transients detected by the Vera C. Rubin Observatory. The instrument is designed with eight parallel channels corresponding to the standard g, r, i, z, Y, J, H, and Ks passbands. Here we present an update on the status of the instrument, the data reduction software, and the current path forward to completion.
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