Current Status of the Lulin Observatory Hung-Chin Lin ( 林宏欽 ), Wen-Ping Chen ( 陳文屏 ), K. H. Chang ( 張光祥 ), Ming-Hsin Chang (張明新), Yung-Hsin Chang (張永欣),

Slides:



Advertisements
Similar presentations
4D2U theater at NAOJ 4D Digital Universe Project Today & Future
Advertisements

Optical monitoring and time delay determination in the gravitationally lensed quasar UM673 E. Koptelova (1,2), V. Oknyanskij (2), B. Artamonov (2), W.-P.
 A telescope collects light coming off an object, like the moon, planets, and stars.  It focuses the light and magnifies it, making the object appear.
What is the AOP? An IFAS approved program for all amateur astronomers Program open to all –Location –Equipment –Knowledge and experience Does not necessarily.
CESAR Educational Astronomy. Objective CESAR (Cooperation through Education in Science and Astronomy Research) will provide students all throughout Europe.
Taken to Ireland for examination and research. The project required substantial financial support, part of which was obtained from the Belfast and Dublin.
Introduction of Lulin Sky Survey (LUSS) T. C. Yang 1, Q. Ye 2, H. C. Lin 1, C. S. Lin 1, W. H. Ip 1 1 Institute of Astronomy, National Central University,
Philip Diamond RadioNet Co-ordinator University of Manchester Jodrell Bank Observatory.
Observations of Active Galactic Nuclei via a Student Operated Remote Observatory Whitney Wills Michael Carini-Faculty Mentor Department of Physics and.
MACQUARIE UNIVERSITY, DEPARTMENT OF PHYSICS RESEARCH – ASTRONOMY & ASTROPHYSICS CORE Astronomy and astrophysics research has grown rapidly at Macquarie.
The Green Bank Telescope a powerful instrument for enhancing ALMA science Unblocked Aperture Low sidelobes gives high dynamic range Resistance to Interference.
Science Team Management Claire Max Sept 14, 2006 NGAO Team Meeting.
Current Status of Lulin Observatory Hung-Chin Lin Taiwan.
Transient Science with the Allen Telescope Array Geoff Bower Berkeley.
OIR Astronomy in Taiwan Wen-Ping Chen NCU/Astronomy Program March 18, 2005 STAR & TELESCOPE XI.
The Path to NGAO Core Science Requirements Claire Max and Liz McGrath NGAO Team Meeting September 11-12, 2008.
China’s Future Missions in Space High Energy Astrophysics Shuang Nan Zhang 张双南 Tsinghua University and Institute of High Energy Physics, Chinese Academy.
The Next 25(?) Years Future Missions to Search for Extra-solar Planets and Life.
KDUST Supernova Cosmology
Observing Facilities of Taiwan and in the Neighborhood Wen-Ping Chen NCU/Astronomy Program March 21, 2003 STAR & TELESCOPE VIII.
January 24, 2006Astronomy Chapter 5 Astronomical Instruments How do we learn about objects too far away for spacecraft? How do telescopes work? Do.
RR Lyraes RR Lyraes are variable stars, which means their apparent brightness as seen from Earth varies. Their intrinsic brightness is around 0.75 and.
Undergraduate Research Experiences at BGSU Presented by Katie Guldenschuh & Andy Layden BRAVO BG! Orlando Florida February 2005.
Undergraduate Research Experiences at BGSU Presented by Katie Guldenschuh & Andy Layden BRAVO BG! Orlando Florida February 2005.
The KPNO 4m “Mayall” Telescope Arjun Dey (NOAO). National Optical Astronomy Observatory Mission: provide the best ground-based astronomical capabilities.
Introducing Astronomy Education into High School Physics Curriculum Through the Use of the University of North Dakota Observatory Caitlin Nolby Space Studies.
Research Performance Ranking of Universities in Taiwan Prof. Ru-Jer Wang Department of Education, Graduate Institute of Educational Policy & Administration,
The Faulkes Telescopes: A Robotic Telescope Network for School Science Students Dr David Frew Department of Physics, Faculty of Science, Macquarie University.
Stars and Cells Kathy Cooksey Astronomy Overview.
GOES Users’ Conference The Role of Geostationary Satellites in WMO’s Global Observing System Dr. Donald E. Hinsman Senior Scientific Officer WMO Satellite.
1 R. D. Gehrz 66th International Symposium on Molecular Spectroscopy, Columbus, OH, June 23, 2011 The Stratospheric Observatory for Infrared Astronomy.
Sternberg Astronomical Institute of Lomonosov Moscow State University.
Telescopes World Tour 2005, continued…. (1888) Near San Jose, CA James Lick made money in real estate Lick telescope a real pyramid… 36-inch Lick Obs.
Our Mission The OPTICON Integrated Infrastructure Initiative brings together all of Western Europe's owners and operators of large observatories and data.
EA ARC Ken Tatematsu East-Asian ARC Manager. ARC organization Difference between ARCS: NA: concentrated in Charlottesville Europe: distributed in different.
The Close Binary Central Star of the Young Planetary Nebula HB12 C. H. Hsia a, W. H. Ip a, J.Y. Hu b a Institute of Astronomy, National Central University,
(Radio) Astronomy in Taiwan Jeremy Lim Institute of Astronomy & Astrophysics, Academia Sinica (ASIAA), Taiwan Taiwan (22.5 million) Malaysia (23 million)
High Energy Gamma Ray projects at the Institute of Space Sciences (ISS) The efforts made at the Institute of Space Sciences in Bucharest to open the VHE.
F. Genova, Berlin 7, Paris, 2 December 2009 The astronomical information network.
European small and medium sized telescopes Paul Murdin Particle Physics & Astronomy Research Council.
Development of space weather in Japan Hiroaki Isobe Center for the Promotion of Interdisciplinary Education and Research Kyoto University.
Report from Subaru Advisory Committee The main issues of the current SAC: ・ Extensive (strategic) program of Subaru telescope ・ International collaborations.
星網計劃 The NETS Project: The NEtwork of Transit Survey 江瑛貴 Ing-Guey Jiang National Tsing-Hua Univ., Taiwan.
TMT.PMO.PRE REL011 Thirty Meter Telescope Background and Status.
A Modern Vision: Eric Lindsay at Armagh Observatory Srividya Subramanian and John McFarland A Modern Vision: Eric Lindsay at Armagh Observatory Srividya.
Swift/BAT Census of Black Holes Preliminary results in Markwardt et al ' energy coded color.
1 R. D. Gehrz 67th International Symposium on Molecular Spectroscopy, Columbus, OH, June 21, 2012 The Stratospheric Observatory for Infrared Astronomy.
The North American ALMA Science Center North America’s ALMA Regional Center The North American ALMA Science Center acts as the gateway to ALMA for North.
1 ASTRONET Coordinating strategic planning for European Astronomy.
Advanced Technologies in Education Virtual Observatory 1 Virtual Observatory: D-Space Project Athens, 14 November 2004 Elena Tavlaki Head of Research Programs.
The Taiwanese-American Occultation Survey (TAOS) Matthew Lehner ASIAA.
Monitor of all-sky X-ray Image (MAXI) was designed to be capable of monitoring variability of a medium-sized sample of active galactic nuclei. As of November.
Wide Field Astronomy from Space Steven Beckwith Space Telescope Science Institute January 9, 2002.
From Pan-STARRS to PTF Wing-Huen Ip Institutes of Astronomy and Space Sciences National Central University Nov. 25, 2011 Sun-Moon Lake, Taiwan.
X-ray sky survey of bright, serendipitous sources with 2XMMi at the AIP Speaker: Alexander Kolodzig Origin: Humboldt-Uni Berlin, Germany Institute:AIP.
1 Preserving and Archiving Astronomical Photographic Plates M. W. Castelaz, J. D. Cline 206 th Meeting of the American Astronomical Society Session
High Energy Astrophysics in Taiwan Hsiang-Kuang Chang ( 張 祥光 ) Department of Physics and Institute of Astronomy National Tsing Hua University ( 國立清華大學.
Status Report of Taiwan Two Meter Telescope Yi Chou Graduate Institute of Astronomy National Central University 2016/1/ 兩岸天文儀器會議.
GBT Future Instrumentation Workshop Fixing the frequency coverage hole in C-Band Jagadheep D. Pandian Cornell University.
Department of Energy Office of Science  FY 2007 Request for Office of Science is 14% above FY 2006 Appropriation  FY 2007 Request for HEP is 8% above.
Compaign of PHEMU Participation of Astronomical Society of Tunis (S.A.T) Tunisia Hanadi Ettroudi Sofien Kamoun H..ETTROUDI,S.A.TAstrometry after.
DEPARTMENT OF PHYSICS AND ASTRONOMY X-ray Astronomy and Space Instrumentation I3 Meeting, December 2004 Integrating Space Radiation Sensing Infrastructures.
AERONET DRAGON Campaign, Summer 2011 Christina Justice College Park Scholars – Science & Global Change Program Environmental Science and Policy
10 January 2006AAS EVLA Town Hall Meeting1 The EVLA: A North American Partnership The EVLA Project on the Web
The Submillimeter Array 1 David J. Wilner
Pentti Pulkkinen Programme Manager Academy of Finland Research funding and administration in Finland
Before, you learned Objects in the universe are grouped together in different ways The motions of planets and other nearby objects are visible from Earth.
Berlin Observatory Berlin, Germany. What is it? The Berlin Observatory is a series of observatories and related organizations in and around the city of.
Graduate Institute of Astronomy National Central University
A Submillimeter and CMBR Observatory for the South Pole
Presentation transcript:

Current Status of the Lulin Observatory Hung-Chin Lin ( 林宏欽 ), Wen-Ping Chen ( 陳文屏 ), K. H. Chang ( 張光祥 ), Ming-Hsin Chang (張明新), Yung-Hsin Chang (張永欣), Zhi-Wei Zhang ( 張智威 ), J. S. Shi ( 石俊雄 ), and J. C. Du (杜進全) Institute of Astronomy, National Central University No. 300, Jung-Da Rd., Jung-Li City, Tao-Yuan, Taiwan 320, R.O.C. Introduction The NCU (National Central University) LuLin Observatory is located at Mt. Front LuLin, 120 o 52' 25" E and 23 o 28' 07" N, a 2862-m peak in the Yu-Shan National Park. The construction of first observatory was finished on January 14, The initial study of LuLin site was started since late Later on, a three-year project was founded by the National Science Council (NSC) to support the development of a modern seeing monitor for this site survey study from 1990 through The average seeing of LuLin site is about 1.39 arc-second. The sky background of this site is mag/arcsec 2 in V band and mag/arcsec 2 in B band. With a 4-year funding supported by the MoE and NSC Excellency project, the NCU has built up the facilities at the LuLin Observatory. This effort, which is coordinated by the Institute of Astronomy of the National Central University, focus on the road construction, water and power supplies, communication links and other items necessary for the establishment and maintenance of the Lu-Lin Observatory as an inter-university astronomical facility for research and education. Abstract After more than ten years of development, the Lulin Observatory is now a full-fledged scientific compound for astronomical observations and other experiments. Among the scientific activity, the Lulin One-meter Telescope (LOT) sees its first light in September The Taiwan-America Occultation Survey (TAOS) telescope array is about to begin routine operation. The Lulin Emission-Line Imaging Survey (LELIS) has started its observing queue. This paper overviews the current status of the site, its operation and management, and future planning at the Lulin Observatory. LOT vs. VLT A very nice galaxy that is called like this due to its stunning appearance. All the tiny little stars around the galaxy are globular clusters. There is a very good photograph (to our knowledge the best earthbound photograph of this galaxy) made with the VLT telescope. We think that our image compares very well with this image regarding the fact that the 1m LOT has cost much less than 1/100 of the VLT cost. Reference Chen W.P., Tsay W.S., Lemme C., Wang J. H., "Taiwan-American Occultation Survey", National Science Council Monthly, Vol. 27 No. 5, May Tsay W.S. et. al., (1999) "The NCU Lu-Lin Observatory and its Future Direction", Proceedings of Fourth East-Asian Meeting on Astronomy, Supplement 1999, p24. Astro Optik Homepage, The Lulin One-meter Telescope (LOT) The Lulin One-meter Telescope (LOT) is the newest and largest telescope in Taiwan. LOT is equipped with the latest scientific instruments for astronomical imaging. The imaging cameras employ highly sensitive arrays of electronic detectors. LOT's purpose is to advance all aspects of Taiwan ground based astronomical research and to provide our best ground-based astronomical telescope to the nation's astronomers, to promote public understanding and support of science. Observing time of LOT is allocated on a seasonal base, January-March (I), April-June (II), July-September (III), and October-December (IV). The major LOT telescope scientific observations in 2003 are as follows, 1.Low-mass X-ray Binary monitoring program 2.Photometric observations of Jovian Trojans 3.Variability of Middle-Aged Open Clusters 4.Photometric Monitoring of Galactic Open Clusters 5.The Morphology and Environment of Seyfert Galaxies Acknowledge This work would not have been possible without the effort of a lot of people working on developing the site. We wish to thank the long term supporting from the National Science Council of Taiwan, the Ministry of Education of Taiwan and the National Central University. Future Development As an inter-university astronomical facility for research and education, members currently involved in this joint venture are Central University (which is operating the Lu-Lin Observatory), Tsinghua University and Taiwan University, but we have the vision that many more universities will be included in this consortium in the near future. We believe that the proposed national infrastructure will promote Taiwan's role in many first-class astronomical projects-from solar system astronomy to cosmology--in view of its capability to provide key longitudinal and time coverage. The Lulin Observatory Control Center (LOCC) The Lulin Observatory Control Center (LOCC) is funded by the MoE and NSC Excellency project and operated by the Institute of Astronomy, National Central University. LOCC operates one major nighttime telescope – LOT, hosts the facilities of consortia. As a national facility, LOCC’s telescopes are open to all astronomers regardless of institutional affiliation. M104 Courtesy Philipp Keller and the LOT team Observing hours statistic in the first season of 2003 A nightly report system is created since 14 Jan Now we have the actual observing hours every night to estimate the weather condition of Lulin site. The total observing hours from 1-Jan to12-Apr is hours. (hr)