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Titlebook: Astrometry of Fundamental Catalogues; The Evolution from O Hans G. Walter,Ojars J. Sovers Book 2000 Springer-Verlag Berlin Heidelberg 2000

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發(fā)表于 2025-3-21 19:18:05 | 只看該作者 |倒序瀏覽 |閱讀模式
期刊全稱Astrometry of Fundamental Catalogues
期刊簡稱The Evolution from O
影響因子2023Hans G. Walter,Ojars J. Sovers
視頻videohttp://file.papertrans.cn/164/163577/163577.mp4
發(fā)行地址Due to powerful computers and the internet there is a change of paradigm taking place in astrometry.The authors, collaborators in the Hipparcos mission, present a final and definitive description of t
學(xué)科分類Astronomy and Astrophysics Library
圖書封面Titlebook: Astrometry of Fundamental Catalogues; The Evolution from O Hans G. Walter,Ojars J. Sovers Book 2000 Springer-Verlag Berlin Heidelberg 2000
影響因子Celestial fundamental catalogues are a prerequisite for the determination of absolute positions and motions in space. Presently, positional astrometry is at the watershed between classical fundamental catalogues, based on moving reference stars, and modern catalogues, based on extragalactic reference objects with non-measurable motion. This book addresses the concepts and methods of the respective construction techniques leading to the stellar frame of the FK5 (fifth fundamental catalogue) and to the newly adopted extragalactic radio reference frame, ICRF (international celestial reference frame), with its extension to optical wavelengths by the Hipparcos Catalogue. While principal outlines of meridian circle observations are given, emphasis is put in some detail on the VLBI technique as applied to astrometry, and to the observational techniques used in the Hipparcos mission, including the tie of the originally non-anchored rigid Hipparcos sphere into the ICRF.
Pindex Book 2000
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發(fā)表于 2025-3-21 22:43:13 | 只看該作者
The Conventional Fundamental Catalogue FK5,on of a fundamental system of positions and proper motions of the stars. Utmost efforts are made to arrive at a catalogue of star positions that represents an inertial frame. The immediate purpose of the catalogue is to serve as the reference frame of positional astronomy. It should also fulfill the
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Astrometry with Radio Interferometers,on of the technique of radio interferometry to the measurement of positions of sources at cosmological distances. With this target in mind we briefly introduce the scope of radio astronomy, followed by a short outline concerning the basic terms and concepts of radio interferometry. We discuss the si
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發(fā)表于 2025-3-22 08:51:39 | 只看該作者
Fundamental Catalogues of Extragalactic Radio Sources,e advantages of an extragalactic system rest, first, upon the observed positions of extragalactic objects (EGOs) whose rotation, when averaged over a large number of objects, would be representative of the rotation of the Universe, which, however, is assumed to be zero according to the discussion in
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The International Celestial Reference Frame: ICRF, belongs to the category of conventional fundamental catalogues. It does not differ fundamentally from the numerous radio catalogues produced during the preceding two decades. This catalogue is merely another member of the category of reference frames produced by the `observable method’ discussed in
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Future Prospects,s employed for connecting observables and their mathematical representation. Accordingly, the associated reference frame and catalogue of celestial objects, which represents the system, are transient products adopted for some interval of time. Typical of this development of a system is the FK5 refer
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