R. Sharp,1 D. Adams,1 G. Bloxham,1 R. Boz,1 D. Bundy,1 D. Chandler,1 G. Gausachs,1 L. Gers,1 J. Hart,1 N. Herrald,1 J. Nielsen,1 E. O'Brien,1 C. Onken,1 I. Price,1 A. Vaccarella,1 C. Vest,1 P. Younghttps://orcid.org/0000-0002-2565-19641
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We report the design evolution for the GMT Integral Field Spectrograph, (GMTIFS). To support the range of operating modes – a spectroscopic channel providing integral field spectroscopy with variable spaxel scales, and a parallel imaging channel Nyquist sampling the LTAO corrected field of view - the design process has focused on risk mitigation for the demanding operational tolerances. We summarise results from prototype components, confirming concepts are meeting the necessary specifications. Ongoing review and simulation of the scientific requirements also leads to new demonstrations of the science that will be made possible with this new generation of high performance AO assisted instrumentation.
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R. Sharp, D. Adams, G. Bloxham, R. Boz, D. Bundy, D. Chandler, G. Gausachs, L. Gers, J. Hart, N. Herrald, J. Nielsen, E. O'Brien, C. Onken, I. Price, A. Vaccarella, C. Vest, P. Young, "Design evolution of the Giant Magellan Telescope Integral Field Spectrograph, GMTIFS," Proc. SPIE 10702, Ground-based and Airborne Instrumentation for Astronomy VII, 107021V (6 July 2018); https://doi.org/10.1117/12.2313010