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Titlebook: Astronomy with Schmidt-Type Telescopes; Proceedings of the 7 Massimo Capaccioli Conference proceedings 1984 D. Reidei Publishing Company, D

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發(fā)表于 2025-3-21 17:52:06 | 只看該作者 |倒序瀏覽 |閱讀模式
期刊全稱Astronomy with Schmidt-Type Telescopes
期刊簡稱Proceedings of the 7
影響因子2023Massimo Capaccioli
視頻videohttp://file.papertrans.cn/164/163655/163655.mp4
學(xué)科分類Astrophysics and Space Science Library
圖書封面Titlebook: Astronomy with Schmidt-Type Telescopes; Proceedings of the 7 Massimo Capaccioli Conference proceedings 1984 D. Reidei Publishing Company, D
影響因子The idea of holding a colloquium on Schmidt telescopes (techniques and science) originated from the observation that, in the last ten years and in spite of the remarkable developments and achievements in this field of astronomical research, there had been no specific opportunity for the experts to meet together, make the point on the state of the art, discuss and coordinate future plans. Therefore, Prof. L. Rosino, one of the pioneers in the use of wide-field telescopes, driven also by the wish of honouring the over four decades of activity of the Asiago Observatory, proposed to the Executive Committee of the International Astronomical Union to sponsor a colloquium on ‘Astronomy with Schmidt type telescopes I to be held at Asiago at the end of the summer of 1983. Details about the composition of the Scientific Organizing Committee and the sponsoring organizations are given in Prof. Rosino‘s ‘Welcome to the Participants ? The granting of this proposal was the beginning of a ‘ number of headaches tor the members of the Local Organizing Committee, R. Barbon, F. Ciatti, P. Rafanelli and myself. If, organlzationwise, the colloquium was successful, this is truly due to the generous effor
Pindex Conference proceedings 1984
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Sky Surveys with the UK 1.2m Schmidt Telescope Messrs. Grubb Parsons of Newcastle-upon-Tyne, to the Science and Engineering Research Council (SERC). The completion of commissioning was marked in 1973 by the taking of the first completely successful sky-limited photograph on hypersensitised Eastman-Kodak IIIa-J emulsion, plate J149 of field 416.
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Machine-Processing of Objective-Prism Plates at the Royal Observatory, Edinburghtive-prism plates. This work is in two categories: (i) semi-automated galaxy redshifts, and (ii) automated quasar detection. The galaxy redshifts are used, for example, to determine the radial velocities of clusters, to test cluster membership, to reveal superimposed clusters, and to reveal connecti
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A Faint Galaxy Survey from Cosmos Measures on Deep UKST Platessurvey of galaxies over large areas of sky down to faint limits (B ~ 21.5). Several fields have been examined, and the data are being used to investigate the properties and large-scale projected distribution of galaxies.
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