HARMONI: ELT的首个光谱学:仪器最终设计和定量性能预测

N. Thatte, I. Bryson, F. Clarke, Vanessa Ferraro-Wood, T. Fusco, D. Le Mignant, D. Melotte, B. Neichel, H. Schnetler, M. Tecza, S. Arribas, A. Crespo, Alberto Estrada Piqueras, Miriam García García, M. Pereira Santaella, Javier Piqueras López, J. Blaizot, Nicholas Bouché, D. Boudon, D. Chapuis, E. Daguisé, K. Disseau, Mtthieu Guibert, A. Jarno, A. Jeanneau, F. Laurent, M. Loupias, J. Migniau, L. Piquéras, A. Remillieux, J. Richard, A. Pécontal-Rousset, L. Bardou, M. Close, R. Deshmukh, S. Dimoudi, Marc Dubbledam, D. King, S. Morris, T. Morris, K. O’Brien, L. Staykov, M. Swinbank, M. Townson, E. Younger, M. Accardo, Domingo Avarez Mendez, R. Conzelmann, S. Egner, E. George, F. Gonté, J. Hopgood, D. Ives, L. Mehrgan, E. Mueller, C. Péroux, J. Vernet, Ángel Alonso-Sánchez, Battaglia Giuseppina, M. Cagigas, J. Delgado, Patricia Fernández Izquierdo, Ana Belén Fragoso López, M. García-Lorenzo, E. Hernández Suárez, José Miguel Herreros Linares, E. Joven, R. López, Y. Martín Hernando, E. Mediavilla, A. Monreal, J
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引用次数: 16

摘要

HARMONI是超大望远镜(ELT)的自适应光学辅助近红外和可见光积分场光谱仪。作为第一台光学仪器,它为ELT提供了主力光谱能力。随着项目接近其最终设计审查里程碑,仪器的设计正在完成,组装、集成和测试的计划正在详细制定。我们从用户的角度概述了仪器的功能,总结了仪器的设计,包括操作和校准计划,并简要介绍了特定观测场景的预测性能。该文件还提供了自2015年项目启动以来财团组成及其演变的一些细节。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
HARMONI: first light spectroscopy for the ELT: instrument final design and quantitative performance predictions
HARMONI is the adaptive optics assisted, near-infrared and visible light integral field spectrograph for the Extremely Large Telescope (ELT). A first light instrument, it provides the work-horse spectroscopic capability for the ELT. As the project approaches its Final Design Review milestone, the design of the instrument is being finalized, and the plans for assembly, integration and testing are being detailed. We present an overview of the instrument’s capabilities from a user perspective, provide a summary of the instrument’s design, including plans for operations and calibrations, and provide a brief glimpse of the predicted performance for a specific observing scenario. The paper also provides some details of the consortium composition and its evolution since the project commenced in 2015.
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