Science I Building Observatory (National Central University Observatory)
Introduction of Science I Building Observatory
The Science I BUilding Observatory, which is equipped with modern facilities and techniques, is the first astronomical research observatory in Taiwan.
The Institute of Physics and Astronomy, National Central University was established in 1977. From then on, the building of the Science I Building Observatory was started. The observatory is completed in 1981. The largest telescope (61 cm) at that time, Cassegrain reflective telescope manufractured by Perkin-Elmer company, was setup in the observatory. In 1990, the telescope is equipped with a CCD(Charge Coupled Device) and start the photometric observations for variable stars, stellar clusters, and binary stars.
Because of the development of the Jhong-Li City, the light pollution grew rapldly. Therefore, the National Central University Observatory was not suitable for the research purposes. A new site survey project, which was executed by prof. Wean-Shun Tsay, was started to find a better site for observatories in Taiwan. After the investigations of seeing conditions, climates, and the stability of the air conditions, they found the front mountain of Lulin is one of the excellent site for the construction of the observatory. The Lulin Observatory was built in 1999, then the National Central University Observatory was turned for the purposes of demostration and education.
Publications related to Science I Building Observatory
Journal Paper
- Wu, H. H., "Photographic and spectrographic observations with a reducing camera on the 61 CM NCU telescope", Astrophysics and Space Science, v.118, p.415, 1986
- Hubbard, W. B., Frecker, J. E., Gehrels, J.-A., Gehrels, T., Hunten, D. M., Lebofsky, L. A., Smith, B. A., Tholen, D. J., Vilas, F., Zellner, B., Avey, H. P., Mottram, K., Murphy, T., Varnes, B., Carter, B., Nielsen, A., Page, A. A., Fu, H. H., Wu, H. H., Kennedy, H. D., Waterworth, M. D., Reitsema, H. J., "Results from observations of the 15 June 1983 occultation by the Neptune system", Astronomical Journal, v.90, p.655, 1985
- Dorren, J. D., Fu, H.-H., Wu, H.-H., "Photometry of the Binary Be Star HR 2142 from November 1983 to January 1984", Informational Bulletin on Variable Stars, v.2521, p.1, 1984
- Vilas, F., Hubbard, W. B., Frecker, J. E., Hunten, D. M., Gehrels, T., Lebofsky, L. A., Smith, B. A., Tholen, D. J., Zellner, B. H., Wisniewski, W., Gehrels, J.-A., Capron, B., Reitsema, H. J., Waterworth, M. D., Fu, H. H., Wu, H. H., Avey, H. P., Page, A. A., "Occultations by Pallas (83/5/29) and Neptune (83/6/15) - Preliminary Results", Bulletin of the American Astronomical Society, v.15, p.816, 1983
- Tsay, W.-S., Kuo, H.-J., Chan, P.-C., "a Binary Observing Project on the Ncuo Speckle Interferometer", Journal of the Korean Astronomical Society, v. 29 Supplement,, p.S409, v.29, p.409, 1996
- Tsay, W. S., "The Application of a Speckle Camera on the NCUO 24-Inch Telescope", Bulletin of the American Astronomical Society, v.22, p.1333, 1990
Theses of Institute of Physics and Astronomy, NCU
- 傅學海:光度儀測試與 DDO 光度系統數據分析
- 陳岸立:獵犬座 RS 型雙星的光度研究
- 梁恩山:太陽振盪的電子耦合元件影像觀測
- 黎煥欣:斑點干涉法在中大二十四吋望遠鏡的測試研究
- 曾宏煇:M15 球狀星團核心成員的高解析運動研究
Theses of Institute of Astronomy, NCU
- 劉志軍:The Construction And Optical Alignment of Solar Magnetic Field Telescope
- 楊曄群:疏散星團 NGC7789 在 UBV 頻帶之光度分析研究 (蔡文祥 指導)
- 詹佩菁:雙星軌道的觀測及統計分析 (蔡文祥 指導)
- 陳炳志:北河二雙星系統在大氣擾動研究上的應用 (蔡文祥 指導)
- 何至誠:太陽磁像儀系統的建構與雜訊分析 (闕志鴻 指導)
- 郭慧君:中大散斑干涉儀於雙星軌道位置之研究 (蔡文祥 指導)
- 李瑾:NGC7790 疏散星團光度觀測研究 (蔡文祥 指導)
- 陳宗楓:應用月掩星技術測量星球角直徑 (陳文屏 指導)
- 吳智雄:行星狀星雲形態之多光譜波段觀測
Thesis of Institute of Earth Sciences, NTNU
- 黃慧春:球狀星團之光度分佈曲線
