Poster + Paper
18 July 2024 G@M: coupling the G-CLEF spectrograph to the Magellan Telescope
Author Affiliations +
Conference Poster
Abstract
G-CLEF is a high-resolution, stabilized, fiber-fed spectrograph designed for the GiantMagellan Telescope (GMT). Before its deployment on the GMT, the instrument will be coupled to the Magellan Clay telescope for several years – the G@M phase. While the spectrograph does not require any modifications, a newly developed interface is required to couple G-CLEF to the telescope. G@M will provide four seeing-limited observing modes and one AO observing mode with the Magellan MagAO-X platform. The design of the seeing-limited front-end unit ensures efficient injection of target, sky/background, and calibration light into the optical fibers. This unit is complemented by additional submodules within the fiber run, incorporating slicing and scrambling capabilities to support extreme precision radial velocity measurement and extreme resolution modes.
(2024) Published by SPIE. Downloading of the abstract is permitted for personal use only.
Yahel Sofer Rimalt, Sagi Ben-Ami, Andrew Szentgyorgyi, Ofir Hershko, Alex Bichkovsky, Enrico Segre, Mark Mueller, Cem Onyuksel, Colby Jurgenson, William Podgorski, Laird Close, and Jared Males "G@M: coupling the G-CLEF spectrograph to the Magellan Telescope", Proc. SPIE 13096, Ground-based and Airborne Instrumentation for Astronomy X, 130964N (18 July 2024); https://doi.org/10.1117/12.3018660
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KEYWORDS
Telescopes

Beam path

Mirrors

Sensors

Spectrographs

Analog to digital converters

Calibration

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