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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Masayuki Miyasaka,Kiyoshi Takatsu the various sections are needed in the quantitative astrophysics of galaxies, globular star clusters, and other extended objects. The methods used come from the morphological characterization of the objects. The ellipse best-fit of isophotes is used for objects, like galaxies, that approximate the

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Pathophysiology of Chronic Kidney Disease completely understandable are noted by (?), while various inclusions for the continuity of the text are indicated by [ ]. The slides and viewgraphs presented in the panel are added as Figures and Tables.]

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Vonda K. Douglas MD,Raul C. Braylan MDand put heavy requirements on the data analysis capability of the ST ScI. This paper presents the general strategy used in ST-related S/W development, and the S/W coordination between the ST Sci and other institutions.

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