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Classical cosmological tests for galaxies of the Hubble Ultra Deep Field

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Abstract

Images of the Hubble Ultra Deep Field are analyzed to obtain a catalog of galaxies for which the angular sizes, surface brightness, photometric redshifts, and absolute magnitudes are found. The catalog contains a total of about 4000 galaxies identified at a high signal-to-noise ratio, which allows the cosmological relations angular size—redshift and surface brightness-redshift to be analyzed. The parameters of the evolution of linear sizes and surface brightness of distant galaxies in the redshift interval 0.5–6.5 are estimated in terms of a grid of cosmological models with different density parameters (Ω V ; Ω m ). The distribution of photometric redshifts of galaxies is analyzed and possible superlarge inhomogeneities in the radial distribution of galaxies are found with scale lengths as large as 2000 Mpc.

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Correspondence to N. V. Nabokov.

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Original Russian Text © N.V. Nabokov, Yu.V. Baryshev, 2008, published in Astrofizicheskij Byulleten, 2008, Vol. 63, No. 3, pp. 260–275.

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Nabokov, N.V., Baryshev, Y.V. Classical cosmological tests for galaxies of the Hubble Ultra Deep Field. Astrophys. Bull. 63, 244–258 (2008). https://doi.org/10.1134/S1990341308030048

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  • DOI: https://doi.org/10.1134/S1990341308030048

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