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2.4m望远镜曝光时间计算器的设计和实现 被引量:1

An Exposure Time Calculator for the 2.4m Telescope of the Yunnan Observatory
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摘要 望远镜的曝光时间计算器对于远程观测以及不熟悉整个观测系统的观测人员尤为重要,因为它可以帮助观测者制定合理的观测计划。设计并实现了高美古2.4m望远镜系统的曝光时间计算器(exposuretimecalculator,ETC),它可以根据望远镜及其终端设备的参数,通过计算给出待测天体曝光时间的参考值。这为观测者了解现有条件下极限观测能力,设置曝光时间或者是给定星等和曝光时间计算信噪比提供了依据。将ETC计算结果与实际测光标准星的数据进行了比较,结果表明ETC对测光标准星的计算结果是可靠的。 Currently,many foreign observatories provide the exposure time calculators(ETCs) for their observational systems,while few people carry out such work in China.An ETC is important for the observers who are unfamiliar with the observational system to plan for observations.The ETC of the 2.4m telescope at the Gaomeigu Station of the Yunnan observatory can give a referential value about the needed exposure based on the parameters of telescope and instruments.Observers can know the feasibility of the desired observations,determine the optimal exposures,or estimate the signal-to-noise ratios(SNRs) of objects according to the given values.From the comparison with the photometric data of standard stars,we have found the results of our ETC to be reliable.
出处 《天文研究与技术》 CSCD 2010年第3期253-260,共8页 Astronomical Research & Technology
关键词 曝光时间 信噪比 测光 Exposure Signal-to-noise ratio Photometry
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  • 1http ://www. na. astro. it/-rifatto/vst/vocet_2, htm#section% 201.
  • 2http ://www. cfht. hawaii. edu/Instruments/Imaging/Megacam/dietmegacam, html#UI.
  • 3ROBERT C. SMITH Observational Astrophysics [M]. CAMBRIDGE.
  • 4Bendinelli. on the determination of Moffit's PSF shape Parameters [ J ]. J Astrophys Astr, 1988, 9:17-24.
  • 5Steven B Howell. two-dimentional aperture photometry: singal-to-noise ratio of point-source observations and optimal data-extraction techniques [ J ]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 1989, 101 : 616 -622.
  • 6http ://www. astro. utoronto. ca/-patton/astro/mags. html.
  • 7ARLO U. LANDOLT. UBVRI PHOTOMETRIC STANDARD STARS IN THE MAGNITUDE 11.5 <V <16. 0 AROUND THE CELESTRIAL EQUATOR [J]. 1992AJ 104... 340L.
  • 8万峰科技.JSP网站开发四酷全书[M].北京:电子工业出版社,2006.

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  • 1国家天文台.SONG中国标准节点望远镜系统方案设计任务书[M].北京:国家天文台,2006.
  • 2Anton Norup Sorensen.SONG general optical layout and functions:SONG-TRE-3400-0047[M].US:[s.n],2009.
  • 3FRIED D L.Probability of getting a lucky short exposure image through turbulence[J].Optical Society of America Journal,1978,68:1651-1658.
  • 4CUI Xiang-qun,SU Ding-qiang,LI Guo-ping,et al.Experiment system of LAMOST active optics[J].SPIE,2004,5489:974-985.
  • 5SU Ding-qiang,JIANG Sheng-tao,ZHOU Wei-yao,et al.Experiment system of thin-mirror active optics[J].SPIE,1982,2199:609-621.
  • 6SU Ding-qiang,ZOU Wei-yao,ZHANG Zhen-chao,et al.Experiment system of segmented-mirror active optics[J].SPIE,2000,4003:417-425.

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