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Observing modes for the new SCORPIO imager and spectrograph at Gemini South

Authors :
Ernesto Sánchez-Blanco
Todd J. Veach
Jason L. Stange
Ronnie Killough
M. Maldonado
Amanda J. Bayless
Kelly D. Smith
Peter W. A. Roming
Alexander J. van der Horst
Marísa Luisa García-Vargas
K. B. Persson
S. Pope
Massimo Robberto
Antonina Brody
Source :
Ground-based and Airborne Instrumentation for Astronomy VII.
Publication Year :
2018
Publisher :
SPIE, 2018.

Abstract

SCORPIO (Spectrograph and Camera for Observation of Rapid Phenomena in the Infrared and Optical) is the new workhorse instrument for the Gemini South Telescope in Chile. Originally proposed in response to the Gen4#3 solicitation, SCORPIO is a unique fast-multicolor imager and ultra-wide band spectrograph capable of rapid exposures for high time-resolution images and spectra. SCORPIO consists of 8 separate channels (corresponding to the standard wavebands g, r, i, z, Y, H, J, K ) that can operate with different exposure times. Each channel can be used in imaging or long-slit mode, with independent readout timing. In this report we illustrate the detectors, the control systems, and the observing modes that will be available with SCORPIO.

Details

Database :
OpenAIRE
Journal :
Ground-based and Airborne Instrumentation for Astronomy VII
Accession number :
edsair.doi...........df7f3be305d8fa39ba08ecd1ead0d320