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Titlebook: Data Analysis in Astronomy; V. Di Gesù,L. Scarsi,S. Levialdi Book 1985 Springer Science+Business Media New York 1985 X-ray.algorithms.astr

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楼主: ergonomics
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Masayuki Miyasaka,Kiyoshi Takatsu is usually a small fraction of the total population. A wide presentation of the method for the “outsiders” can be found in Diaconis and Efron (1983) and Efron (1982). Also see Simpson (1984, this volume).
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The Data Analysis Facilities that Astronomers Wantthey need, particularly in the U.K. Although my views are coloured by my recent experiences in setting up and running STARLINK I should point out that they are not the official views of that project, from which I have now retired. This talk is collected under the following headings:
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Time Analysis in Astronomy: Tools for Periodicity Searchesst Fourier Transform, Rayleigh Test, Epoch Folding) are reviewed with the main objective to compare cost and sensitivities in different applications. One of the main results of the discussion is that FFT procedures are convenient in unbiased searches for periodicity in radio astronomy, while in spar
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Graphical Methods of Exploratory Data Analysiswest of a family of “Prim” systems whose most striking common feature is the use of real-time motion graphics to display three-dimensional scatterplots. Orion I differs from earlier Prim systems through the use of modern and relatively inexpensive raster graphics and microprocessor technology. It al
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Faint Objects in Crowded Fields: Discrimination and Countingcularly relevant in the case of crowded regions. The density of the object images can be evaluated by comparing the distribution of the object dimensions with the distribution of the distances between any object and its nearest neighbor. We refer to the case in which the modes of the two distributio
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