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Published in: Measurement Techniques 3/2013

01-06-2013

A cosmological distance scale program

Author: A. N. Klenitskii

Published in: Measurement Techniques | Issue 3/2013

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Abstract

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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Literature
1.
go back to reference M. Humason, N. Mayall, and A. Sandage, “Red shift and magnitudes of extragalactic nebulae,” Astronom. J., 61, 97 (1956).ADSCrossRef M. Humason, N. Mayall, and A. Sandage, “Red shift and magnitudes of extragalactic nebulae,” Astronom. J., 61, 97 (1956).ADSCrossRef
2.
go back to reference W. K. Freedman et al., “Final results from the Hubble space telescope key project to measure the Hubble constant,” Astrophys. J., 553, 47 (2001).ADSCrossRef W. K. Freedman et al., “Final results from the Hubble space telescope key project to measure the Hubble constant,” Astrophys. J., 553, 47 (2001).ADSCrossRef
3.
go back to reference A. G. Riess et al., “A redetermination of the Hubble constant with the Hubble space telescope from a differential distance ladder,” http://arXiv:0905.0695v1[astro-ph.CO], accessed Dec. 15, 2012. A. G. Riess et al., “A redetermination of the Hubble constant with the Hubble space telescope from a differential distance ladder,” http://​arXiv:​0905.​0695v1[astro-ph.CO], accessed Dec. 15, 2012.
4.
go back to reference S. Perlmutter et al., “Measurements of Ω and Λ from 42 high-red shift supernovae,” Astrophys. J., 517, 565–586 (1999).ADSCrossRef S. Perlmutter et al., “Measurements of Ω and Λ from 42 high-red shift supernovae,” Astrophys. J., 517, 565–586 (1999).ADSCrossRef
5.
go back to reference G. Burbidge and M. Burbidge, Quasi-Stellar Objects, W. H. Freeman, San Francisco (1967). G. Burbidge and M. Burbidge, Quasi-Stellar Objects, W. H. Freeman, San Francisco (1967).
6.
go back to reference S. F. Levin, “A cosmological distance scale based on a red shift interpolation model,” Izmer. Tekhn., No. 6, 12–14 (2012); Measur. Techn., 55, No. 6, 609–612 (2012). S. F. Levin, “A cosmological distance scale based on a red shift interpolation model,” Izmer. Tekhn., No. 6, 12–14 (2012); Measur. Techn., 55, No. 6, 609–612 (2012).
7.
go back to reference Yu. S. Vladimirov, A. N. Klenitskii, and V. G. Krechet, “The problem of interpreting the cosmological red shift,” Yarosl. Pedagog. Vestnik, No. 2, 53–62 (2010). Yu. S. Vladimirov, A. N. Klenitskii, and V. G. Krechet, “The problem of interpreting the cosmological red shift,” Yarosl. Pedagog. Vestnik, No. 2, 53–62 (2010).
8.
go back to reference S. F. Levin, “Statistical methods of solving cosmological and gravitational measurement problems,” in: Physics of Fundamental Interactions: Proc. Int. Conf. on Nuclear Physics, OFN Ross. Akad. Nauk, Moscow (2012). S. F. Levin, “Statistical methods of solving cosmological and gravitational measurement problems,” in: Physics of Fundamental Interactions: Proc. Int. Conf. on Nuclear Physics, OFN Ross. Akad. Nauk, Moscow (2012).
9.
go back to reference K. Lang, Astrophysical Formulae, Springer, NY (1999). K. Lang, Astrophysical Formulae, Springer, NY (1999).
10.
go back to reference J. Guy et al., “The supernova legacy survey 3-year sample: Type Ia supernovae photometric distances and cosmological constraints,” Astron. Astrophys., 523, A7 (2010).ADSCrossRef J. Guy et al., “The supernova legacy survey 3-year sample: Type Ia supernovae photometric distances and cosmological constraints,” Astron. Astrophys., 523, A7 (2010).ADSCrossRef
Metadata
Title
A cosmological distance scale program
Author
A. N. Klenitskii
Publication date
01-06-2013
Publisher
Springer US
Published in
Measurement Techniques / Issue 3/2013
Print ISSN: 0543-1972
Electronic ISSN: 1573-8906
DOI
https://doi.org/10.1007/s11018-013-0183-4

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