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TPoint is computer software that implements a mathematical model of conditions leading to errors in telescope pointing and tracking. The model can then be used in a telescope control system to correct the pointing and tracking. Such errors are typically caused by mechanical or structural defects. For example, TPoint can analyze and compensate for systematic errors such as polar misalignment, mechanical and optical non-orthogonality, lack of roundness in telescope mounting drive gears, as well as for flexure of the mounting caused by gravity. TPoint is in use on the majority of professional telescopes worldwide, including the Anglo-Australian Observatory, Keck Observatory, Gemini Observatory, and many others. It has significantly improved the performance and efficiency of telescope operation and has had an especially strong impact on the development of automated and robotic telescopes. TPoint is also widely used by amateur astronomers. Software Bisque distributes TPoint for Windows; this version is used to improve the pointing on amateur telescopes. ==History== TPoint was invented and developed by Patrick Wallace.〔 It grew out of work performed by Patrick Wallace and John Straede at the Anglo-Australian Telescope (AAT) between 1974 and 1980 using Interdata 70 computers. In the early 1980s, it was ported to the Digital Equipment Corporation VAX running under the VMS operating system and between 1990 and 1992 was also ported to run on the PC/MS-DOS platform as well as various UNIX platorms.〔 〕 抄文引用元・出典: フリー百科事典『 ウィキペディア（Wikipedia）』 ■ウィキペディアで「Tpoint」の詳細全文を読む スポンサード リンク
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