Hostname: page-component-586b7cd67f-r5fsc Total loading time: 0 Render date: 2024-11-30T05:40:08.297Z Has data issue: false hasContentIssue false
  • English
  • Français

The NCU Lu-Lin Observatory

Published online by Cambridge University Press:  12 April 2016

Wean-Shun Tsay ,
Alfred Bing-Chih Chen ,
Kuang-Hsiang Chang  and
Huan-Hsin Li
Wean-Shun Tsay
Affiliation:
Institute of Astronomy, National Central University, Chung-Li 32054, Taiwan
Alfred Bing-Chih Chen*
Affiliation:
Institute of Astronomy, National Central University, Chung-Li 32054, Taiwan
Kuang-Hsiang Chang
Affiliation:
Institute of Astronomy, National Central University, Chung-Li 32054, Taiwan
Huan-Hsin Li
Affiliation:
Institute of Astronomy, National Central University, Chung-Li 32054, Taiwan
*
1 Current Address: Department of Physics, National Cheng-Kung University, Tainan 70101, Taiwan

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The NCU (National Central University) Lu-Lin observatory is located at Mt. Front Lu-Lin, 120°52′25”E and 23°28′07” N, a 2862-m peak in the Yu-Shan National Park. The construction of Lu-Lin observatory was finished on January 14, 1999. The initial assessment of Lu-Lin site started in 1989, after which a three-year project was founded by the National Science Council (NSC) to support a modern seeing monitoring program. The average seeing at Lu-Lin is about 1.39 arc-second with an average of 200 clear nights annually. The sky background is 20.72 mag/arcsec2 in V band and 21.22 mag/arcsec2 in B band.

The Lu-Lin observatory is for both research and education. A homemade 76-cm Super Light Telescope (SLT) and four TAOS 50-cm robotic telescopes for a survey on Kuiper Belt Objects will be the two major research facilities. The pilot program for SLT consists of observations of time-varying astrophysical phenomena. The TAOS #1 telescope was installed at Lu-Lin in March 2000. A 90 KW/240 VAC power line and a water pipe system have been pulled to the site in early 2001. A wireless Network system through A-Li Shan has been operating at Lu-Lin observatory while a faster wireless Network system with 11.5 Mbit/sec bandwidth is under consideration and may be available in the near future for remote observing.

Type
VII. Science With Small Telescopes
Information
International Astronomical Union Colloquium , Volume 183: Small-Telescope Astronomy on Global Scales , 2001 , pp. 299 - 303
Copyright
Copyright © Astronomical Society of the Pacific 2001

References

Ardeberg, A. 1987, in “Identification, Optimization, and Protection of Optical Telescope Sites”, Proc. of an International Conf. Flagstaff, AZ Google Scholar
Fried, D.L. 1965, J. Opt. Soc. Am., 55, 1427 CrossRefGoogle Scholar
Fried, D.L. 1966, J. Opt; Soc. Am., 56, 1372 Google Scholar
King, S.K. 2001, this volumeGoogle Scholar
Tsay, W.S. et al. 1999, in ” The NCU Lu-Lin Observatory and its Future Direction” , Proceedings of Fourth East-Asian Meeting on Astronomy, 1999, p24 Google Scholar
Woolf, N.J. 1982, ARA&A, 20, 367 Google Scholar