Astrometry and photometry of asteroids from the UkrVO database of astroplates

I. Vavilova, S. Shatokhina, L. Pakuliak, O. Yizhakevych, I. Eglitis, V. Andruk, Y. Protsyuk
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引用次数: 3

Abstract

Abstract We present the developed methods of digitization, image processing, reduction, and scientific data mining with the latest reference catalogs, which allowed us to obtain a good positional and photometric accuracy in B-band of 6,500 asteroids down to 17.5 m from the Ukrainian Virtual Observatory database of astroplates. The archive includes FON-Kyiv, FON-Kitab, FON-Dushanbe sky surveys (1981–1996) and astroplates of the Baldone and Tautenburg observatories. For some of asteroids, observations are either completely absent or not enough over the certain time interval to the moments of their official discoveries (about 300 such objects were found). Positional observations during these time scales are highly useful for a more detailed study of the dynamics and orbital parameters of asteroids as well as the obtained photometric parameters are very complementary with present-day data for studying changes in brightness and light curves.
来自UkrVO星盘数据库的小行星天体测量和光度测定
摘要利用最新的参考星表,采用数字化、图像处理、约简和科学数据挖掘等方法,从乌克兰虚拟天文台星盘数据库中获得了6500颗小于17.5 m的小行星的b波段定位和光度精度。档案包括基辅天文台、基塔布天文台、杜尚别天文台的天空调查(1981-1996)和巴尔多内天文台和陶滕堡天文台的星盘。对于一些小行星,要么完全没有观测,要么在它们正式发现的那一刻(大约发现了300个这样的天体)的一定时间间隔内观测不足。在这些时间尺度上的位置观测对于更详细地研究小行星的动力学和轨道参数非常有用,并且获得的光度参数与目前研究亮度和光曲线变化的数据非常互补。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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