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OIR Astronomy in Taiwan

This document discusses the astronomical infrastructures in Taiwan, Japan, Korea, and China. It highlights various observatories including Taiwan's SMART/SMA, AMiBA, and Lulin One-meter Telescope, as well as significant institutions such as AURA and AUI. The aim is to showcase how these countries are enhancing their capabilities in astronomical observation and research through collaboration and advanced facilities. With a focus on organization and management, it emphasizes the importance of international partnerships in achieving scientific advancements in astronomy.

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OIR Astronomy in Taiwan

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  1. OIR Astronomy in Taiwan Wen-Ping Chen NCU/Astronomy Program March 18, 2005 STAR & TELESCOPE XI ST11@NTU

  2. National Infrastructure Possible Models --- • Observing Facilities, e.g., NOAO • Managing Consortium, e.g., AURA • Umbrella Organization, e.g., NAOJ, NAOC ST11@NTU

  3. AURA (Association of Universities for Research in Astronomy) AURA is a consortium of universities, and educational and other non-profit institutions, that operates world-class astronomical observatories that we term "centers." Our members are 30 U.S. institutions and 6 international affiliates. We view ourselves as acting on behalf of the science communities that are served by our centers, and as trustees and advocates for the centers' missions. ST11@NTU

  4. AUI (Associated Universities, Inc.) X Associated Universities, Inc., (AUI) is a not-for-profit corporation based in Washington, DC. It was founded in 1946 by nine northeastern universities to manage major scientific facilities. AUI currently operates the National Radio Astronomy Observatory under a cooperative agreement with the National Science Foundation. ST11@NTU

  5. More --- Government Buffering Agents • Some make sense …DoE  national labs, e.g., MIT  Lincoln Lab UC  Lawrence Livermore Lab  Los Alamos Lab U Chicago  Argonne Lab • Some less obvious …NASA operates centers, e.g., GSFC, directlybut Caltech  JPL? ST11@NTU

  6. Japan • Nobeyama（野邊山）millimeter 45 m dish + array (10 m x 6) • Okayama（岡山）(1.88 m) • Subaru (8 m), e.g., 1.3 m IRSF at SAAO Nagoya U) ST11@NTU

  7. Korea • Bohyunsan Obs (1.8 m) • Taeduk Radio Ast Obs (TRAO, 45 m) • KVN (Korean VLBI Network) + Japanese VLBI • GALEX (Galaxy Evolution Explorer) UV imaging/spectroscopyhttp://www.srl.caltech.edu/galex/ • 4 astronomy/space science journals ST11@NTU

  8. China • BAO (2.16 m, 60/90 Schmidt); ShAO (1.56 m) • Seshan (25 m); Urumqi (25 m) • LAMOST (Large Sky Area Multi-Object Fiber Spectroscopic Telescope)4 m; 4000 fibers; v~20.5 mag in 1.5 hrs, with 1 nm res www.lamost.org • SST (Space Solar Telescope) 1m; res 0.1” • Re-infrastructured … ST11@NTU

  9. Taiwan • SMART/SMA (Sub-Millimeter Array)(6m x 8; baseline 8-508 m; 180-900 GHz) • AMiBA (1.2m/0.3m x 19; on a 6 m fully steerable platform; 90 GHz) really an experiment • TAOS (0.5 m x 4) • LOT (Lulin One-meter Telescope) • TON (Taiwan Oscillation Network) • TEN (Taiwan Earth-Shine Network) • Maidanak 1 m ST11@NTU

  10. How the neighbors are looking ahead? • China BAO 興隆 1 m + LAMOST… Yunnan Obs 2.3 m OIR at Gaomeigu 高美古 PMO 盱眙 1.2/1.0 m Schimidt for NEOs • Korea 1.8 m  Mexican 6.5 m x 2? • Pan-Asia 2.5 m IR telescope (site?) • Japan Okayama 1.88 m  3.5 m (?) Buying time on 2-4 m world-wide ST11@NTU

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