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The Influence of the Peculiar Velocities of SNe Ia in Clusters of Galaxies on the Redshift Measurements

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Abstract

The most intriguing question of modern astronomy is the question of our Universe formation. The Hubble diagram analysis with Type Ia Supernovae (SNe Ia) is widely used to estimate the cosmological parameters with high accuracy. The cosmological measurements allow us to better understand the early stages of the Universe evolution. Nevertheless, the redshift on the SN Ia Hubble diagram includes the contribution from the unknown peculiar velocities that decreases the accuracy of such measurements. We consider the contamination of peculiar velocities of the host galaxies for those SNe that exploded in galaxy clusters. For this purpose, we use the Pantheon cosmological sample and offer the procedure to minimize the influence of such uncertainties.

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ACKNOWLEDGMENTS

The authors are grateful to Pierre-Francois Léget for the helpful discussion. This work has made use of data from the Sloan Digital Sky Surveys [19] and the SIMBAD database, operated at CDS, Strasbourg, France [21].

Funding

E.A.B. and M.V.P. acknowledge support from RSF grant 18-72-00159 and the Interdisciplinary Scientific and Educational School of Moscow University “Fundamental and Applied Space Research”.

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Authors and Affiliations

  1. Lomonosov Moscow State University, Faculty of Physics, 119991, Moscow, Russia

    E. A. Balakina

  2. Lomonosov Moscow State University, Sternberg Astronomical Institute, 119234, Moscow, Russia

    E. A. Balakina & M. V. Pruzhinskaya

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  1. E. A. Balakina
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  2. M. V. Pruzhinskaya
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Correspondence to E. A. Balakina or M. V. Pruzhinskaya.

Additional information

Paper presented at the Fourth Zeldovich meeting, an international conference in honor of Ya.B. Zeldovich held in Minsk, Belarus, on September 7–11, 2020. Published by the recommendation of the special editors: S.Ya. Kilin, R. Ruffini, and G.V. Vereshchagin.

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Balakina, E.A., Pruzhinskaya, M.V. The Influence of the Peculiar Velocities of SNe Ia in Clusters of Galaxies on the Redshift Measurements. Astron. Rep. 65, 897–901 (2021). https://doi.org/10.1134/S1063772921100012

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