Graduate Institute of Astronomy National Central University

Slides:



Advertisements
Similar presentations
Welcome to the University of Michigan – Dearborn Observatory Founded 2007.
Advertisements

Astronomical works with students Irina GUSEVA St Petersburg - Central (Pulkovo) Astronomical Observatory of the Russian Academy of Sciences - St Petersburg.
GTN The GLAST Telescope Network Involvement for students and teachers in the science of the Swift, GLAST, and XMM-Newton missions Gordon Spear and Tim.
Building the Sonoma State University Robotic Telescope
CESAR Educational Astronomy. Objective CESAR (Cooperation through Education in Science and Astronomy Research) will provide students all throughout Europe.
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,
Observations of Active Galactic Nuclei via a Student Operated Remote Observatory Whitney Wills Michael Carini-Faculty Mentor Department of Physics and.

M77 (NGC 1068) By: Ryan Desautels. Messier 77 A Brief History A Brief History General Information General Information Galactic Information Galactic Information.
Fan Zhou Profs Jun Ma and Xu Zhou BATC Group,NAOC The BATC Multicolor Photometric Study of M31 Globular Clusters.
Current Status of Lulin Observatory Hung-Chin Lin Taiwan.
Brian Schmidt, Paul Francis, Mike Bessell, Stefan Keller.
TOPS 2003 Remote Obs 1 Karen Meech Institute for Astronomy TOPS 2003 Image copyright, R. Wainscoat, IfA Image courtesy K. Meech.
The MACHO Experiment Aishwarya Bhake Astronomy 007: Big Bang and Beyond 4/13/2006.
_______________ RIT Observatory Data Pipeline & Automation Project: Summer Research ______________________ Presented by: Kevin Beaulieu & Dustin Crabtree.
INSTRUMENTATION AT THE GETTYSBURG OBSERVATORY….And what to do with it. American Astronomical Society 205 th meeting, San Diego, Jan 13, 2005.
Adding TDI mode to PRISM Li Zeng Advisor: Brian Taylor Jan.25, 2008.
X-ray sources in NSVS Tim McKay University of Michigan 04/03/04.
Observing. Next Tuesday We’ll meet at the observatory even if it is cloudy –If the weather is really bad (a foot of snow or something) I’ll send an .
The Nearby Supernovae Factory: Spectrograph Calibration Ben Dilday Advisor: Rick Kessler, CfCP Physics 335 Autumn 2003.
The Faulkes Telescopes: A Robotic Telescope Network for School Science Students Dr David Frew Department of Physics, Faculty of Science, Macquarie University.
Agile: A Time-Series CCD Photometer to Study Variables Anjum Mukadam, Russell Owen, Ed Mannery University of Washington, Seattle.
Searching for Meaning in the Universe 在宇宙中尋找存在的意義 Credit: Gary Tonge.
MONGOLIAN-RUSSIAN COOPERATION IN KHURELTOGOOT OBSERVATORY IN THE ISON PROJECT FRAMEWORK N.Tungalag 1, I.Molotov 2, V.Voropaev 2, V.Kouprianov 3, Yu.Krugly.
July Light pollution map. If interested in astronomy, the last place you want to be is in the Northeast.
Weidong Li Jesse Leaman Alex Filippenko Department of Astronomy University of California, Berkeley Nearby Supernova Rates from the Lick Observatory Supernova.
Sternberg Astronomical Institute of Lomonosov Moscow State University.
Amateur Astronomy The Bangalore Astronomical Society ®
Research and Imaging Program for the SVAS. Current Situation Society supports beginners well –Messier Group –Community Outreach programs Monthly star.
The Chinese SONG proposal: scientific concerns Jianning Fu (Beijing Normal University) and Chinese SONG team Beijing ─ March 29, 2010 The third workshop.
Nyrölä Observatory Petri Tikkanen Jyväskylän Sirius ry.
Studies Of Galaxy Clusters By BATC Large Field Multi-Color Sky Survey --- A brief review of the progresses in recent years Yanbin, Yang; Xu, Zhou BATC,
星網計劃 The NETS Project: The NEtwork of Transit Survey 江瑛貴 Ing-Guey Jiang National Tsing-Hua Univ., Taiwan.
Database of Variable Stars Bingqiu Chen Dept of Astronomy Beijing Normal University.
Subaru/FMOS Commissioning: Brief history & current status Naoyuki Tamura Instrument scientist Subaru Telescope, NAOJ Expected performance Observation “A.
Northern Prairie Star Party
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),
The Taiwanese-American Occultation Survey (TAOS) Matthew Lehner ASIAA.
Wide Field Astronomy from Space Steven Beckwith Space Telescope Science Institute January 9, 2002.
© Sierra College Astronomy Department 1 Astronomy 10 Elementary Astronomy COURSE GOALS & OBJECTIVES.
Prepare your scantron: Please take a moment to mute your cell phone!
Long Term Monitoring of AGNs with Bell Astrophysical Observatory Whitney Wills Western Kentucky University Advisor: Dr. Michael Carini.
PHEMU The Bucharest observational campaign Romanian Astronomical Institute of The Romanian Academy - AIRA ADRIAN SONKA, MARCEL POPESCU, DAN ALIN.
Discussion: Summary & Questions. Specification of 2m space station UV/Op telescope D : Aperture 2m f / D 12 focal lenth 24m Field view : 1.5 degree Final.
GALAXIES IN THE FIELD OF THE GAMMA-RAY BURST GRB I.V. Sokolov, Yu.V. Baryshev, T.A. Fatkhullin Results (counts of galaxies, photometric red shifts,
(there’s no place like home) The Milky Way Galaxy.
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.
MMT Observation Database for Light Curve Analysis Vladimir Agapov Presentation for the WG1 session 33rd IADC meeting, Houston.
The Robotic Liverpool Telescope Dr. Chris Leigh 1 st September 2011 Astrophysics Research Institute Liverpool John Moores University Discover the Cosmos.
EXPLORE/OC: Photometry Results for the Open Cluster NGC 2660 K. von Braun (Carnegie/DTM), B. L. Lee (Toronto), S. Seager (Carnegie/DTM), H. K. C. Yee (Toronto),
Status of LAMOST ZHAO Yongheng National Astronomical Observatories of China.
Remote observatory ISON-NM Survey of Minor Solar System bodies L. Elenin¹, I. Molotov¹, V. Savanevich², A. Kozhukhov³, A. Bryukhovetskiy³, V. Vlasenko³,
VISTA Visible and Infrared Survey Telescope for Astronomy Spring Semester // Giant Telescope Sciences April 12 th. Youkyung Ko.
The Reduction and Reporting of Data On Proto-Planetary Nebulae From Two Observatories. By Wesley Cheek With Mr. Wen Lu & Prof. Bruce Hrivnak.
GCSE Astronomy.
V. Agapov, N. Sakva, D.Davydov, E.Katkova
Using a Radio Telescope
Presented by: Kevin Beaulieu & Dustin Crabtree
Prepare your scantron:
X Serbian-Bulgarian Astronomical Conference (X SBAC)
Telescopes.
Amy Meadows NGC 3718.
University of Leicester Observatories
Chapter 12 Supernova Remnant

WFCAM Photometric Calibration
The Commissioning of Northern Arizona University’s Barry Lutz Telescope Student Arron Shiffer Mentor S.C. Tegler.
UCAC U.S. Naval Observatory CCD Astrograph Catalog T.J. Rafferty
Telescopes & Instrumentation

Presentation transcript:

Graduate Institute of Astronomy National Central University Current Status of Lulin Observatory and of the One-Meter Telescope: Operation and Management H. C. Lin & M. H. Chang Graduate Institute of Astronomy    National Central University

LOT Lulin One-meter Telescope (LOT) 2002/09 – Installation, Alignment 2002/10 ~12 – Test Observing 2003/01 – Time Allocation

LOT Cassegrain optics Fork type equatorial mount D=1,000mm f.l.=8,000mm Fully Computer Control

Performance Pointing~ 1’ RMS Tracking (no guiding)~300sec Limiting Mag. ~19 , Merr=0.1 (R-band, exptime=60sec)

NGC1278 field (AP8 ccd, R-band, exp300s )

Limiting Magnitude of Field SA92 by Dr. Alfred Chen (AP8 ccd, R-band, exp60s )

Instrumentation CCD: AP-8/FLI IMG1024S (f.o.v.~10.6’x10.6’, 0.62” x 0.62”/pixel) Filters: B/V/R/H-alpha/R Continuum After April 2003… New CCD: Princeton Instruments 1300B (f.o.v.~11’x11’, 0.52” x 0.52”/pixel) New Filter Wheel: B/V/R/I/H-alpha/OIII/SII/R Continuum …14 filters

Test Observation Total Observing time~ 300hrs(2002/9-11) Asteroid light curve Asteroid discovery: Lulin1 (2002WT18) X-ray binary, Open cluster, Supernovae Engineering Time: Seeing condition, Pointing Model, Tracking, Guiding…

Lulin Site Seeing ~1.39 ” ,best seeing<1.0” (1993) Sky background: 21.22 mag/arcsec^2 (B-band), 20.72 mag/arcsec^2 (V-band) (1994)

Time Allocation TAC: 7 (NCUx5, NTHUx1, NCKUx1) 4 TA/year: I(Jan.-Mar.), II(Apr.-Jun.), III(Jul.-Sep.), IV(Oct.-Dec.) Observing Proposal Require (http://www.astro.ncu.edu.tw)

2003I TA 1. X光新星中的Superhump現象與軌道週期之研究與高質量X-射線雙星的光學確認 2. Low-mass X-ray Binary monitoring program 3.X-ray binaries和Cataclysmic variables的光度曲線分析 4. Photometric observations of Jovian Trojans 5. The study of morphology in large size halos surrounding planetary nebulae 6. Variability of Middle-Aged Open Clusters 7. Photometric Monitoring of Galactic Open Clusters 8. The Morphology and Environment of Seyfert Galaxies