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

Modeling of giant radio galaxy distribution over the sphere in the millimeter-wavelength range 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. http://www.deepdyve.com/assets/images/DeepDyve-Logo-lg.png Astrophysical Bulletin Springer Journals

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

Astrophysical Bulletin , Volume 72 (3) – Sep 9, 2017

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Publisher
Springer Journals
Copyright
Copyright © 2017 by Pleiades Publishing, Ltd.
Subject
Physics; Astronomy, Astrophysics and Cosmology
ISSN
1990-3413
eISSN
1990-3421
DOI
10.1134/S1990341317030117
Publisher site
See Article on Publisher Site

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.

Journal

Astrophysical BulletinSpringer Journals

Published: Sep 9, 2017

References