Optical sky brightness at Dome A, Antarctica, from the Nigel experiment

Nigel is a fiber-fed UV/visible grating spectrograph with a thermoelectrically-cooled 256×1024 pixel CCD camera, designed to measure the twilight and night sky brightness from 300nm to 850 nm. Nigel has three pairs of fibers, each with a field-of-view with an angular diameter of 25 degrees, pointing...

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Bibliographic Details
Published in:SPIE Proceedings, Ground-based and Airborne Telescopes III
Main Authors: Sims, Geoff, Ashley, Michael C B, Cui, Xiangqun, Everett, Jon R., Feng, Long Long, Gong, Xuefei, Hengst, Shane, Hu, Zhongwen, Lawrence, Jon S., Luong-Van, Daniel M., Shang, Zhaohui, Storey, John W V, Wang, Lifan, Yang, Huigen, Yang, Ji, Zhou, Xu, Zhu, Zhenxi
Other Authors: Stepp, Larry M., Gilmozzi, Roberto, Hall, Helen J.
Format: Other Non-Article Part of Journal/Newspaper
Language:English
Published: SPIE 2010
Subjects:
Online Access:https://researchers.mq.edu.au/en/publications/e45e43ab-28d1-43d0-816b-a70a8f8dea4c
https://doi.org/10.1117/12.857795
https://research-management.mq.edu.au/ws/files/62456108/Publisher%20version%20(open%20access).pdf
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