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Chinese Small Telescope ARray (CSTAR) for Antarctic Dome A

机译:中国南极半球小型望远镜ARray(CSTAR)

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Chinese first arrived in Antarctic Dome A in Jan. 2005 where is widely predicted to be a better astronomical site thanDome C where have a median seeing of 0.27arcsec above 30m from the ground. This paper introduces the first Chinese Antarctic telescope for Dome A (CSTAR) which is composed of four identical telescopes, with entrance pupil 145 mm, 20 square degree FOV and four different filters g, r, i and open band. CSTAR is mainly used for variable stars detection, measurement of atmosphere extinction, sky background and cloud coverage. Now CSTAR has been successfully deployed on Antarctic Dome A by the 24th Chinese expedition team in Jan. 2008. It has started automatic observation since March 20, 2008 and will continuously observe the south area for the whole winter time. The limited magnitude observed is about 16.5~m with 20 seconds exposure time. CSTARS's success is a treasurable experience and we can benefit a lot for our big telescope plans, including our three ongoing 500mm Antarctic Schmidt telescopes (AST3).
机译:中国人于2005年1月首次到达南极穹顶A,在这里,人们普遍认为它比天文学的天文学家更好。 圆顶C,离地面30m处的中位数为0.27arcsec。本文介绍了第一台中国南极A型穹顶望远镜(CSTAR),它由四个相同的望远镜组成,它们的入射光瞳为145 mm,视场角为20平方度,并具有四个不同的滤光镜g,r,i和开放波段。 CSTAR主要用于可变恒星检测,大气消光,天空背景和云层覆盖的测量。现在,CSTAR已于2008年1月由第24中国探险队成功部署在南极穹顶A上。自2008年3月20日起,它已开始自动观测,并将在整个冬季持续观测南部地区。暴露时间为20秒时,观察到的有限量级约为16.5μm。 CSTARS的成功是宝贵的经验,我们可以从我们的大型望远镜计划中受益匪浅,其中包括三架正在进行中的500mm南极施密特望远镜(AST3)。

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