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Titlebook: Science with the VLT Interferometer; Proceedings of the E Francesco Paresce Conference proceedings 1997 Springer-Verlag Berlin Heidelberg 1

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書(shū)目名稱Science with the VLT Interferometer
副標(biāo)題Proceedings of the E
編輯Francesco Paresce
視頻videohttp://file.papertrans.cn/863/862615/862615.mp4
概述This is an outlook for future research..Based on such conferences proposals for actual observations are worked out by scientists.
叢書(shū)名稱ESO Astrophysics Symposia
圖書(shū)封面Titlebook: Science with the VLT Interferometer; Proceedings of the E Francesco Paresce Conference proceedings 1997 Springer-Verlag Berlin Heidelberg 1
描述It has always been ESO‘s aim to operate the VLT in an interferometric mode (VLTI) which allows the coherent combination of stellar light beams col- lected by the four 8-m telescopes and by several smaller auxiliary telescopes. In December 1993, in response to financial difficulties, the ESO Council de- cided to postpone implement at ion of the VLTI, Coude trains and associated adaptive optics for all the UTs but included provisions for continuing tech- nological and development programmes devoted to the aim of reintroducing these capabilities at the earliest possible date. The desirability of carrying out the full VLTI programme as originally envisaged at the earliest possible moment has not, however, diminished, es- pecially in view of VLTI‘s exceptional capabilities and resulting potential for new and exciting discoveries. In recent years, interferometric projects have begun to playa central role in ground-based high-resolution astronomy, and numerous instruments have been completed or are in the process of construc- tion. Several large-aperture interferometers will probably co me on-line near the turn of the century. The impending presence of these new instruments represents an
出版日期Conference proceedings 1997
關(guān)鍵詞Population; active galactic nuclei; astrometry; astronomy; cosmology; extrasolar planet; galaxy; interferom
版次1
doihttps://doi.org/10.1007/978-3-540-69398-7
isbn_softcover978-3-662-22399-4
isbn_ebook978-3-540-69398-7Series ISSN 1431-2433 Series E-ISSN 1611-6143
issn_series 1431-2433
copyrightSpringer-Verlag Berlin Heidelberg 1997
The information of publication is updating

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Introduction to Interferometry and closure phase, which can then be fitted by a model or used to reconstruct an image. In order to measure fringes, the path lengths from the source to the detector via the different individual apertures must be equalized. This requires some form of fringe tracking, which constrains the type of ob
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Astrometry with Optical/IR Interferometerssed interferometers: global astrometry and narrow angle astrometry. The ultimate limits for both types of measurements are set by the atmosphere. However, the instrumental considerations for the two types of measurements are quite different. This paper gives an overview of the instrumental aspects o
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Solar-System Observations with the VLTIs (from 0.3 AU to more than 50 AU). VLTI observations of Solar-system objects will concentrate on targets with angular dimensions in the range of an arcsec or smaller. Major objectives are expected to be the search for asteroid companions, the morphological study of asteroids, satellites of outer pl
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