SOXS 的可见光探测器系统
天体物理仪器与方法
2018-09-06 v1
摘要
SOXS 将是 ESO NTT 望远镜上独一无二的光谱设施，凭借两条不同臂覆盖光学与近红外波段：UV-VIS（350–850 nm）与 NIR（800–1800 nm）。本文描述可见光相机低温恒温器的设计及采集系统的架构。UV-VIS 探测器系统基于 e2v CCD 44-82、与 ESO 连续流低温恒温器（CFC）冷却系统及 ESO 开发的 NGC CCD 控制器耦合的定制探测器头。本文概述该系统现状并描述构成 UV-VIS 臂的各部件设计，并附有一系列描述 SOXS 设计方案的投稿。
引用
@article{arxiv.1809.01570,
title = {The VIS detector system of SOXS},
author = {Rosario Cosentino and Matteo Aliverti and Salvatore Scuderi and Sergio Campana and Riccardo Claudi and Pietro Schipani and Andrea Baruffolo and Sagi Ben-Ami and L. H. Mehrgan and Derek Ives and Federico Biondi and Anna Brucalassi and Giulio Capasso and Francesco D'Alessio and Paolo D'Avanzo and Oz Diner and Hanindyo Kuncarayakti and Matteo Munari and Adam Rubin and Fabrizio Vitali and Jani Achren and Jose Antonio Araiza-Duran and Iair Arcavi and Andrea Bianco and Enrico Cappellaro and Mirko Colapietro and Massimo Della Valle and Sergio D'Orsi and Daniela Fantinel and Johan Fynbo and Avishay Gal-Yam and Matteo Genoni and Mika Hirvonen and Jari Kotilainen and Tarun Kumar and Marco Landoni and Jussi Lehti and Gianluca Li Causi and Luca Marafatto and Seppo Mattila and Giorgio Pariani and Giuliano Pignata and Michael Rappaport and Davide Ricci and Marco Riva and Bernardo Salasnich and R. Zanmar Sanchez and Stephen Smartt and Massimo Turatto},
journal= {arXiv preprint arXiv:1809.01570},
year = {2018}
}
备注
9 pages, 13 figures, to be published in SPIE Proceedings 10702