Poster
6 June 2024 Design, assembly, and test of G-CLEF's exposure meter I: design trade-off and first conclusions
Author Affiliations +
Conference Poster
Abstract
This project aims to formulate, design , build and test a versatile, high-efficiency, low-resolution spectrograph to function as the G-CLEF (GMT-Consortium Large Earth Finder) exposure meter. G-CLEF, the first-generation Giant Magellan Telescope's (GMT) instrument, is a state-of-the-art, high-resolution, echelle spectrograph for the GMT, expected to be completed for the telescope's first light. The exposure meter plays a vital role for adjusting barycentric corrections of Doppler radial velocity (RV) by accounting for t Earth's chromatic atmospheric influences. Its significance becomes pronounced in Extreme Precision RV (EPRV) measurements, where the atmosphere's wavelength dependency contributes to errors at the scale of tens of centimeters per second, the same level of precision required for detecting Earth-analog planets orbiting stars similar to the Sun, aligning with one of the primary scientific objectives of G-CLEF. This paper explores the scientific motivation in detail, describes the designs trade-off analysis and the performance simulations aiming to achieve 1cm/s precision on EPRV measurements and outlines the resulting principal parameters derived from these analyses.
(2024) Published by SPIE. Downloading of the abstract is permitted for personal use only.
Henrique Lupinari, Sagi Ben-Ami, Rafael Ribeiro, Claudia Mendes de Oliveira, and Andrew Szentgyorgyi "Design, assembly, and test of G-CLEF's exposure meter I: design trade-off and first conclusions", Proc. SPIE 13024, Optical Instrument Science, Technology, and Applications III, (6 June 2024); https://doi.org/10.1117/12.3028567
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KEYWORDS
Design

Earth atmosphere

Precision measurement

Spectrographs

Telescopes

Equipment

Planets

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