New reduction of old glass astronomical plates of Pallas and Vesta in 1956-1994 based on Gaia DR3 catalogue

被引:1
|
作者
Wang, L. L. [1 ]
Yu, Y. [1 ,2 ]
Yuldoshev, Q. X. [3 ]
Ehgamberdiev, Sh. A. [3 ,4 ]
Shang, Z. J. [1 ]
Yang, M. T. [1 ]
Yang, J. [1 ]
Dong, S. [1 ]
Da, D. M. [1 ]
Tang, Z. H. [1 ,2 ]
Zhao, J. H. [1 ]
Muminov, M. M. [3 ]
机构
[1] Chinese Acad Sci, Shanghai Astron Observ, Shanghai, Peoples R China
[2] Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing 100049, Peoples R China
[3] Uzbek Acad Sci, Ulugh Beg Astron Inst, Tashkent 100052, Uzbekistan
[4] Natl Univ Uzbekistan, Tashkent 100174, Uzbekistan
基金
中国国家自然科学基金;
关键词
Astrometry; Asteroids; general; Methods; observational;
D O I
10.1016/j.pss.2023.105637
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Through a key project for intergovernmental international cooperation between Uzbekistan and China, a group of old glass astronomical plates of Pallas and Vesta taken by the TAS033 telescope at Tashkent observation site of Ulugh Beg Astronomical Institute in 1956-1994 have been digitized using the digitizer with sub-micrometer measuring precision newly developed by Shanghai Astronomical Observatory. Based on the Gaia DR3 cata-logue, a new reduction of these old observations was carried out. A total of 105 Pallas and 83 Vesta astrometric positions were derived. The comparison with theoretical values from JPL ephemerides indicates that the dispersion of the positions of Pallas from the digitized plates are better than 0.1300 in both right ascension and declination, and the dispersions of the positions of Vesta are better than 0.2100.
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页数:6
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