Astrometric and photometric observations of six brightest trans-Neptunian objects at the Kyiv comet station

IF 0.2 Q4 ASTRONOMY & ASTROPHYSICS Advances in Astronomy and Space Physics Pub Date : 2021-07-06 DOI:10.17721/2227-1451.10.40-54
A. Baransky, O. Lukina, S. Borysenko
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Abstract

In this work we focused on observations of six trans-Neptunian objects (TNOs) whose apparent magnitudes are brighter than 20m. We present the results of astrometric and photometric observations of (134340) Pluto, (136108) Haumea, (136472) Makemake, (136199) Eris, (90482) Orcus, and (20000) Varuna obtained at the Kyiv comet station (Code MPC 585) in 2017-2019. For observations we used the 0.7-m (f/4) reflector AZT-8 with FLI PL4710 CCD camera and filters of Johnson-Cousins photometric system. From our images we measured the objects' astrometric positions, calculated apparent magnitudes in the BVRI (mostly R) bands using aperture photometry method, and found absolute magnitudes together with the colour indices in several bands. Analysing our results, we investigate the limitation on the astrometry and photometry of faint objects with the 0.7-m telescope.
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在基辅彗星站对六个最亮的海王星外天体进行天文测量和光度观测
在这项工作中,我们重点观察了六个视星等超过20米的跨海王星天体。我们介绍了2017-2019年在基辅彗星站(代码MPC 585)获得的(134340)冥王星、(136108)豪美阿、(136472)马克马克、(136199)伊利斯、(90482)奥库斯和(20000)瓦鲁纳的天体测量和光度观测结果。为了进行观测,我们使用了0.7-m(f/4)反射器AZT-8和FLI PL4710 CCD相机以及Johnson Cousins光度系统的滤光片。根据我们的图像,我们测量了物体的天体测量位置,使用孔径测光法计算了BVRI(主要是R)波段的视星等,并在几个波段找到了绝对星等和颜色指数。通过分析我们的结果,我们研究了0.7米望远镜对微弱物体的天体测量和光度测定的限制。
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Advances in Astronomy and Space Physics
Advances in Astronomy and Space Physics ASTRONOMY & ASTROPHYSICS-
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