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CCD整体平差方法的FORTRAN语言归算程序
引用本文:于涌,李金岭,唐正宏,赵铭.CCD整体平差方法的FORTRAN语言归算程序[J].中国科学院上海天文台年刊,2005(1):110-118.
作者姓名:于涌  李金岭  唐正宏  赵铭
作者单位:中国科学院上海天文台,中国科学院上海天文台,中国科学院上海天文台,中国科学院上海天文台 上海 200030,上海 200030,上海 200030,上海 200030
基金项目:中国科学院知识创新工程(KJCL2-SW-TI)、国家自然科学基金(No.10333050,No.10173019,No.10473019)项目资助课题.
摘    要:介绍了实现CCD整体平差的FORTRAN归算程序的详细流程,包括(a)数据收集、(b)预处理和(c)整体平差与结果输出共三个步骤,并给出了各步所调用的子程序名称及其功能说明。采用模拟数据对该程序进行了可靠性检验,并将该程序应用于4颗河外射电源的光学定位。结果表明, 由于利用整体平差方法参加归算的观测资料覆盖天区扩大,包含了较多的参考星,因而可以获得高于单底片归算的定位精度。

关 键 词:天体测量  数据分析  参考系
收稿时间:2005-01-13
修稿时间:2005-04-06

A FORTRAN REALIZATION OF THE BLOCK ADJUSTMENT OF CCD FRAMES
YU Yong, TANG Zhenghong ,LI Jinling ,ZHAO Ming.A FORTRAN REALIZATION OF THE BLOCK ADJUSTMENT OF CCD FRAMES[J].Annals of Shanghai Observatory Academia Sinica,2005(1):110-118.
Authors:YU Yong  TANG Zhenghong  LI Jinling  ZHAO Ming
Affiliation:Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030
Abstract:A FORTRAN version realization of the block adjustment (BA) of overlapping CCD frames is developed. The flowchart is introduced including (a) data collection, (b) preprocessing, and (c) BA and object positioning. The subroutines and their functions are also demonstrated. The program package is tested by simulated data with/without the application of white noises. It is also preliminarily applied to the reduction of optical positions of four extragalactic radio sources. The results show that because of the increase in the sky coverage and number of reference stars, the precision of deducted positions is improved compared with single plate adjustment.
Keywords:astrometry - methods  data analysis - reference systems
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