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6 July 2018 GMACS: a wide-field, moderate-resolution spectrograph for the Giant Magellan Telescope
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Abstract
We discuss the latest developments of a spectrograph for the Giant Magellan Telescope. The instrument is designed to provide high throughput, moderate resolution, optical spectra for the telescope and be capable of flexible and rapid reconfiguration. The focal plane can be populated with custom slit masks or multiple fibers, allowing for observations of multiple objects simultaneously.
Conference Presentation
© (2018) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
D. L. DePoy, Luke M. Schmidt, Rafael Ribeiro, Keith Taylor, Damien Jones, Travis Prochaska, Jennifer L. Marshall, Erika Cook, Cynthia Froning, Tae-Geun Ji, Hye-In Lee, D. M. Faes, A. Souza, D. Bortoletto, Claudia Mendes de Oliveira, Soojong Pak, and Casey Papovich "GMACS: a wide-field, moderate-resolution spectrograph for the Giant Magellan Telescope", Proc. SPIE 10702, Ground-based and Airborne Instrumentation for Astronomy VII, 107021X (6 July 2018); https://doi.org/10.1117/12.2313940
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