Large Scale Distribution of Galaxies in the Field HS 47.5–22. II. Observational Data Analysis

We present results of the study of the large scale distribution of galaxies up to z ~ 0 . 8 in the field HS 47.5–22 based on the photometric data obtained with the 1 m Schmidt telescope of the Byurakan astrophysical observatory (BAO NAS). The complete sample includes 28 398 galaxies brighter than up...

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Veröffentlicht in:	Astrophysical bulletin 2020-07, Vol.75 (3), p.219-233
Hauptverfasser:	Grokhovskaya, A. A., Dodonov, S. N., Movsesyan, T. A.
Format:	Artikel
Sprache:	eng
Schlagworte:	Adaptive algorithms Astronomy Astrophysics and Cosmology Data analysis Density Galaxy distribution Physics Physics and Astronomy Schmidt telescopes Tessellation
Online-Zugang:	Volltext
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