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Modeling of giant radio galaxy distribution over the sphere in the millimeter-wavelength range

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Abstract

We suggest a method and build a model of radio galaxy distribution over the sphere using data from the WENSS catalogs and standard radio count models by Condon. We calculate the angular power spectrum of the contribution of extended radio galaxies into the microwave background and show that it can be a distorting factor for correct estimation of the angular spectrum from the signal determined by the Sunyaev–Zeldovich effect.

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Authors and Affiliations

  1. St. Petersburg Branch of the Special Astrophysical Observatory of the Russian Academy of Sciences, St. Petersburg, 196140, Russia

    D. I. Solovyov

  2. Special Astrophysical Observatory, Russian Academy of Sciences, Nizhnii Arkhyz, 369167, Russia

    O. V. Verkhodanov

Authors
  1. D. I. Solovyov
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  2. O. V. Verkhodanov
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Correspondence to D. I. Solovyov.

Additional information

Original Russian Text © D.I. Solovyev, O.V. Verkhodanov, 2017, published in Astrofizicheskii Byulleten’, 2017, Vol. 72, No. 3, pp. 239–246.

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Solovyov, D.I., Verkhodanov, O.V. Modeling of giant radio galaxy distribution over the sphere in the millimeter-wavelength range. Astrophys. Bull. 72, 217–223 (2017). https://doi.org/10.1134/S1990341317030117

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  • DOI: https://doi.org/10.1134/S1990341317030117

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