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A cosmological distance scale program

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Measurement Techniques Aims and scope

A program for identifying the cosmological distance scale for different models of the red shift in the spectra of extragalactic sources from the observed red shifts and stellar magnitudes, combined with the database on supernovae, radio galaxies and quasars, is developed. The Friedmann–Mattig and generalized interpolation models in combination with models of the intrinsic red shift of the sources are taken as the main parameters.

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Authors and Affiliations

  1. Lomonosov Moscow State University, Moscow, Russia

    A. N. Klenitskii

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  1. A. N. Klenitskii
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Correspondence to A. N. Klenitskii.

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Translated from Metrologiya, No. 1, pp. 3–7, January, 2013.

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Klenitskii, A.N. A cosmological distance scale program. Meas Tech 56, 223–225 (2013). https://doi.org/10.1007/s11018-013-0183-4

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  • DOI: https://doi.org/10.1007/s11018-013-0183-4

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