Project of program package for exploring of cosmological fractals

The value of fractal dimension and inhomogeneity scale of the spatial distribution of galaxies is a widely discussed problem in the modern cosmology. To solve it one should carefully test the reliability of methods of determination of the values of these physical quantities. The project of a program...

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Бібліографічні деталі
Опубліковано в: :Advances in Astronomy and Space Physics
Дата:2012
Автор: Lovyagin, N.Yu.
Формат: Стаття
Мова:English
Опубліковано: Головна астрономічна обсерваторія НАН України 2012
Онлайн доступ:https://nasplib.isofts.kiev.ua/handle/123456789/119175
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Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Цитувати:Project of program package for exploring of cosmological fractals / N.Yu. Lovyagin // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 1. — С. 63-66. — Бібліогр.: 21 назв. — англ.

Репозитарії

Digital Library of Periodicals of National Academy of Sciences of Ukraine
id nasplib_isofts_kiev_ua-123456789-119175
record_format dspace
spelling Lovyagin, N.Yu.
2017-06-04T18:38:52Z
2017-06-04T18:38:52Z
2012
Project of program package for exploring of cosmological fractals / N.Yu. Lovyagin // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 1. — С. 63-66. — Бібліогр.: 21 назв. — англ.
2227-1481
https://nasplib.isofts.kiev.ua/handle/123456789/119175
The value of fractal dimension and inhomogeneity scale of the spatial distribution of galaxies is a widely discussed problem in the modern cosmology. To solve it one should carefully test the reliability of methods of determination of the values of these physical quantities. The project of a program package to explore fractal properties of isolated points (galaxies) distribution is presented. The package includes tools to load catalogues of galaxies as well as to simulate fractal and uniform distributions of points, which are used for testing applicability limits of correlation methods.
Author is thankful to Y. V. Baryshev and N. K. Kosovsky for their help. The work is partly supported by Russian Foundation for Basic Research, Grant 09-02-00143.
en
Головна астрономічна обсерваторія НАН України
Advances in Astronomy and Space Physics
Project of program package for exploring of cosmological fractals
Article
published earlier
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
title Project of program package for exploring of cosmological fractals
spellingShingle Project of program package for exploring of cosmological fractals
Lovyagin, N.Yu.
title_short Project of program package for exploring of cosmological fractals
title_full Project of program package for exploring of cosmological fractals
title_fullStr Project of program package for exploring of cosmological fractals
title_full_unstemmed Project of program package for exploring of cosmological fractals
title_sort project of program package for exploring of cosmological fractals
author Lovyagin, N.Yu.
author_facet Lovyagin, N.Yu.
publishDate 2012
language English
container_title Advances in Astronomy and Space Physics
publisher Головна астрономічна обсерваторія НАН України
format Article
description The value of fractal dimension and inhomogeneity scale of the spatial distribution of galaxies is a widely discussed problem in the modern cosmology. To solve it one should carefully test the reliability of methods of determination of the values of these physical quantities. The project of a program package to explore fractal properties of isolated points (galaxies) distribution is presented. The package includes tools to load catalogues of galaxies as well as to simulate fractal and uniform distributions of points, which are used for testing applicability limits of correlation methods.
issn 2227-1481
url https://nasplib.isofts.kiev.ua/handle/123456789/119175
citation_txt Project of program package for exploring of cosmological fractals / N.Yu. Lovyagin // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 1. — С. 63-66. — Бібліогр.: 21 назв. — англ.
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