东京大学阿塔卡马天文台6.5m望远镜:斯巴鲁望远镜上近红外仪器SWIMS的对空性能

M. Konishi, K. Motohara, H. Takahashi, N. Kato, Kosuke Kushibiki, Hiroki Nakamura, Nuo Chen, T. Kodama, M. Hayashi, I. Tanaka, K. Tadaki, J. Toshikawa, Y. Koyama, Rhytmh Shimakawa, Tomoko L. Suzuki, T. Asano, H. Okita, S. Koshida, K. Tateuchi, Soya Todo, Y. Kobayakawa, Yutaro Kitagawa, H. Ohashi, Yukihiro Kono, Y. Terao, T. Aoki, K. Asano, M. Doi, B. Hatsukade, T. Kamizuka, K. Kohno, T. Minezaki, T. Miyata, T. Morokuma, Mizuki Mumata, S. Sako, H. Sameshima, T. Soyano, T. Tanabé, Masuo Tanaka, K. Tarusawa, R. Ohsawa, Kengo Tachibana, Tsubasa Michifuji, Y. Yoshii
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引用次数: 7

摘要

同色宽视场红外多目标光谱仪(SWIMS)是东京大学阿塔卡马天文台(TAO) 6.5米望远镜的第一代设施仪器之一,目前正在智利北部Cerro Chajnantor山顶(海拔5640米)建造。SWIMS有两个光学臂,蓝色臂覆盖0.9-1.4µm,红色臂覆盖1.4-2.5µm,通过在准直光束中插入一个二向镜,因此能够在成像模式下同时拍摄两个滤光片波段的图像,或在光谱学(MOS)模式下拍摄整个近红外(0.9-2.5µm)低至中分辨率的多目标光谱,两者都只需要一次曝光。2017年,斯巴鲁6.5米望远镜建成前,将SWIMS送入斯巴鲁望远镜进行性能评估,并于2018年5月成功实现成像首光,2019年1月成功实现MOS首光。经过三次工程运行,包括首次光观测,SWIMS已被接受为斯巴鲁望远镜从S21A学期到S22B学期的新PI仪器。在本文中,我们报告了在总共7.5个晚上的工程观测中评估的仪器的天空性能细节。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
The University of Tokyo Atacama Observatory 6.5m telescope : On-sky performance of the near-infrared instrument SWIMS on the Subaru telescope
The Simultaneous-color Wide-field Infrared Multi-object Spectrograph (SWIMS) is one of the 1st generation facility instruments for the University of Tokyo Atacama Observatory (TAO) 6.5 m telescope currently being constructed at the summit of Cerro Chajnantor (5,640 m altitude) in northern Chile. SWIMS has two optical arms, the blue arm covering 0.9–1.4 µm and the red 1.4–2.5 µm, by inserting a dichroic mirror into the collimated beam, and thus is capable of taking images in two filter-bands simultaneously in imaging mode, or whole nearinfrared (0.9–2.5 µm) low-to-medium resolution multi-object spectra in spectroscopy (MOS) mode, both with a single exposure. SWIMS was carried into Subaru Telescope in 2017 for performance evaluation prior to completion of the construction of the 6.5 m telescope, and successfully saw the imaging first light in May 2018 and MOS first light in Jan 2019. After three engineering runs including the first light observations, SWIMS has been accepted as a new PI instrument for Subaru Telescope from the semester S21A until S22B. In this paper, we report on details of on-sky performance of the instrument evaluated during the engineering observations for a total of 7.5 nights.
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