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—From January 2019 to February 2021, observations of the linear polarization of the object S5 0716+714 were carried out with the Zeiss-600 telescope of SAO RAS. A Felix Savart plate was used as a polaroid. The result is a Fourier power spectrum of the linear polarization variation in the frequency range of \documentclass[12pt]{minimal}\usepackage{amsmath}\usepackage{wasysym}\usepackage{amsfonts}\usepackage{amssymb}\usepackage{amsbsy}\usepackage{mathrsfs}\usepackage{upgreek}\setlength{\oddsidemargin}{-69pt}\begin{document}$$f = 10$$\end{document}–\documentclass[12pt]{minimal}\usepackage{amsmath}\usepackage{wasysym}\usepackage{amsfonts}\usepackage{amssymb}\usepackage{amsbsy}\usepackage{mathrsfs}\usepackage{upgreek}\setlength{\oddsidemargin}{-69pt}\begin{document}$$150$$\end{document} days\documentclass[12pt]{minimal}\usepackage{amsmath}\usepackage{wasysym}\usepackage{amsfonts}\usepackage{amssymb}\usepackage{amsbsy}\usepackage{mathrsfs}\usepackage{upgreek}\setlength{\oddsidemargin}{-69pt}\begin{document}$$^{{ - 1}}$$\end{document} without any harmonic component evidence; the spectrum is proportional to the power law \documentclass[12pt]{minimal}\usepackage{amsmath}\usepackage{wasysym}\usepackage{amsfonts}\usepackage{amssymb}\usepackage{amsbsy}\usepackage{mathrsfs}\usepackage{upgreek}\setlength{\oddsidemargin}{-69pt}\begin{document}$$F \sim {{f}^{{ - 0.55}}}$$\end{document}. The distribution of polarization values over the entire observation period is subject to the Relay distribution which does not demonstrate any signs of a periodic component. There is a harmonic dependence of the polarization on the brightness of an object with a period of 10 mJy.
Astrophysical Bulletin – Springer Journals
Published: Mar 1, 2022
Keywords: BLLacertae: individual: S5 0716+714; techniques: polarimetry; instruments: polarimeters
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