Titlebook: Data Analysis in Astronomy IV; V. Gesù,L. Scarsi,H. U. Zimmermann Book 1992 Springer Science+Business Media New York 1992 astronomy.astrop

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Matthew Davenport,Laura E. Dickinson Ph.D.later the ROSAT telescope began its operation with an observation of the central parts of the Large Magellanic Cloud. This long awaited event marked the begin of a new phase in X-ray astronomy during that an extension of our present database on X-ray sources by an order of magnitude is expected.

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https://doi.org/10.1007/978-1-4684-4826-9 soon replace the IHAP system at ESO’s New Technology Telescope (NTT) when the NTT will be used also under remote control from ESO Headquarters in Garching. Observers will then have all utilities of a modern astronomical data analysis system at their finger tips, at the telescope..This paper describ

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Chronic Venous Disorders of the Lower Limbse form of two-dimensional images of the physical world and consists of measurements which are dependent on factors such as the imaging geometry, illumination, and structures present in the world. The goal of any vision system is to recognize familiar structures in the system’s environment, and obtai

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Jeffrey M. Rhodes,Peter Gloviczkith-independent. It has been used to analyse data from the Einstein Observatory, EXOSAT and Ginga, as well as optical photometry and helioseismology data. In the currently available version (No. 2.0), XRONOS includes programs for: light curve(s), hardness ratio and colour-colour plotting, epoch foldi

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Venous Anatomy of the Lower Limbdge about spacial and kinematical characteristics of stellar populations. The tasks and the present state of the MEGA program has been described recently by Malyuto, Einasto, Kharchenko and Schilbach (1990). The use of absolute proper motions of stars (with respect to galaxies), photoelectric UBVR a