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Titlebook: Data Analysis in Astronomy III; V. Gesù,L. Scarsi,M. C. Maccarone Book 1989 Springer Science+Business Media New York 1989 astronomy.astrop

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发表于 2025-3-21 17:06:42 | 显示全部楼层 |阅读模式
书目名称Data Analysis in Astronomy III
编辑V. Gesù,L. Scarsi,M. C. Maccarone
视频video
丛书名称Ettore Majorana International Science Series
图书封面Titlebook: Data Analysis in Astronomy III;  V. Gesù,L. Scarsi,M. C. Maccarone Book 1989 Springer Science+Business Media New York 1989 astronomy.astrop
描述In the book are reported the main results presented at the Third International Workshop on Data Analysis in Astronomy, held at the EUore Majorana Center for Scientific Culture, Erice, Sicily, Italy, on June 20-27,1988. The Workshop was the natural evolution of the two previous ones. The main goal of the first edition (Erice 1984) was to start a scientific interaction between Astronomers and Computer Scientists. Aim of the second (Erice 1986) was to look at the progress in data analysis methods and dedicated hardware technology. Data analysis problems become harder whenever the data are poor in statistics or the signal is weak and embedded in structured background. Experiments collecting data of such a nature require new and non-standard methodologies. Possibilistic approaches could be merged with the statistical ones, in order to formalize all the knowledge used by the scientists to reach conclusions. Moreover, the last decade has been characterized by very fast developments of Intelligent Systems for data analysis (knowledge based systems, ... ) that would be useful to support astronomers in complex decision making. For these reasons, the last edition of the workshop was intended
出版日期Book 1989
关键词astronomy; astrophysics; cosmic ray; energy; entropy; gravitation; laser; observatory; quasar; radiation; stab
版次1
doihttps://doi.org/10.1007/978-1-4684-5646-2
isbn_softcover978-1-4684-5648-6
isbn_ebook978-1-4684-5646-2
copyrightSpringer Science+Business Media New York 1989
The information of publication is updating

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The Rayleigh Statistic in the Case of Weak Signals — Applications and Pitfallsstrength is less than this limit, then one should be careful when interpreting results, since the bias increases rapidly as p→0 which may result in the possibility of identifying a signal where none exists.
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A Model for the Infrared Space Observatory Photometerrogress regarding the production of this model, in which case we will attempt to make this model as general as possible so that it may be used in modelling other similar experiments. In this paper we will discuss the problems associated with this work, the overall design concept, and the implementation.
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Stability in Factor Analyses with Respect to Small Perturbations of the Data and to Departure from Gond step, we recall the principle of two non-parametric processes, namely jackknife and bootstrap. In a last stage, we compare the robustness of the asymptotic results mentioned earlier with the results obtained through non parametric processes by means of simulation and drawing of random samples in a given population.
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Statistical Restoration of Astronomical Images(i,j) is given by.where ε. represents the external contribution, in our case background and random noise. The main problem in the restoration of astronomical images is to estimate S(,) on a grid of points from the Z values, knowledge of the psf and adequate assumptions about the noise process.
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Multidimensional Discrete Signals Description Using Rotation and Scale Invariant Pattern Spectruma structuring element, called kernel, strategically chosen by the observer. A morphological operation is then constitucd by a transformation followed by some measurement on the transformed signal. The measurement on the transformed signal can be its lenght, area, volume, etc., depending on the dimension of the signal.
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Applications of Decomposition Algorithm in Clustering Methodsto study properties of non-fuzzy partitions derived from a number of algorithms providing convex decomposition of matrix U..We suggest the possibility of the application of decomposition algorithm in clustering methods in two approaches:
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Yukari Shindo,Michiaki Yamakage that the latter is much more adequate to exhibit some periodic terms confirmed in the case of the sun demi-diameter through another analysis of oneothe authors (Laclare, 1985). Furthermore, the increased accuracy of the estimations in the parameters of the relative solar orbit (Bougeard and al 1983) shows that this method is relevant.
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