Email this article Modeling of giant radio galaxy distribution over the sphere in the millimeter-wavelength range
- Authors: Solovyov D.I.1, Verkhodanov O.V.2
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Affiliations:
- St. Petersburg Branch of the Special Astrophysical Observatory of the Russian Academy of Sciences
- Special Astrophysical Observatory
- Issue: Vol 72, No 3 (2017)
- Pages: 217-223
- Section: Article
- URL: https://journals.rcsi.science/1990-3413/article/view/212459
- DOI: https://doi.org/10.1134/S1990341317030117
- ID: 212459
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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.
About the authors
D. I. Solovyov
St. Petersburg Branch of the Special Astrophysical Observatory of the Russian Academy of Sciences
Author for correspondence.
Email: drukhi@ya.ru
Russian Federation, St. Petersburg, 196140
O. V. Verkhodanov
Special Astrophysical Observatory
Email: drukhi@ya.ru
Russian Federation, Nizhnii Arkhyz, 369167
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