Soxs：由于重力屈曲，温度变化和子系统对准引起的光学性能的影响

论文标题

Soxs：由于重力屈曲，温度变化和子系统对准引起的光学性能的影响

SOXS: Effects on optical performances due to gravity flexures, temperature variations, and subsystems alignment

论文作者

Sanchez, Ricardo Zanmar, Aliverti, Matteo, Munari, Matteo, Campana, Sergio, Claudi, Riccardo, Schipani, Pietro, Baruffolo, Andrea, Ben-Ami, Sagi, Biondi, Federico, Capasso, Giulio, Cosentino, Rosario, D'Alessio, Francesco, D'Avanzo, Paolo, Hershko, Ofir, Kuncarayakti, Hanindyo, Landoni, Marco, Pignata, Giuliano, Rubin, Adam, Scuderi, Salvatore, Vitali, Fabrizio, Young, David, Achrén, Jani, Araiza-Duran, José Antonio, Arcavi, Iair, Brucalassi, Anna, Bruch, Rachel, Cappellaro, Enrico, Colapietro, Mirko, Della Valle, Massimo, de Pascale, Marco, di Benedetto, Rosario, D'Orsi, Sergio, Gal-Yam, Avishay, Genoni, Matteo, Hernandez, Marcos, Kotilainen, Jari, Causi, Gianluca Li, Mattila, Seppo, Rappaport, Michael, Radhakrishnan, Kalyan, Ricci, Davide, Riva, Marco, Salasnich, Bernardo, Smartt, Stephen, Stritzinger, Maximilian, Ventura, Hector

论文摘要

Soxs（X-Shooter的儿子）是La Silla的360万New Technology Telescope（NTT）的新型中分辨率宽波光谱仪。 SOXS将提供0.35至2.0μm的同时波长覆盖范围，并专用于瞬时和可变源的研究。虽然先前的程序中介绍了系统的名义光学性能（ARXIV：1809.01521），但我们在这里提出了一系列旨在识别和量化光学效应的进一步分析，这是由于在对齐和操作过程中仪器的温度和方向变化而导致的。

SOXS (Son Of X-Shooter) is the new medium resolution wide-band spectrograph to be installed at the 3.6m New Technology Telescope (NTT) in La Silla. SOXS will offer simultaneous wavelength coverage from 0.35 to 2.0 μm and will be dedicated to the study of transient and variable sources. While nominal optical performances of the system were presented in previous proceedings (arXiv:1809.01521), we here present a set of further analyses aimed to identify and quantify optical effects, due to changes in temperature and orientation of the instrument during alignment and operations.

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