Single-Dish Radio Polarimetry in the F-GAMMA Program with the Effelsberg 100-m Radio Telescope

Studying the variability of polarized AGN jet emission in the radio band is crucial for understanding the dynamics of moving shocks as well as the structure of the underlying magnetic field. The 100-m Effelsberg Telescope is a high-quality instrument for studying the long-term variability of both to...

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Main Authors: Beuchert Tobias, Kadler Matthias, Wilms Jörn, Angelakis Emmanouil, Fuhrmann Lars, Myserlis Ioannis, Nestoras Ioannis, Kraus Alex, Bach Uwe, Ros Eduardo, Grossberger Christoph, Schulz Robert
Format: Article
Language:English
Published: EDP Sciences 2013-12-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/20136106006
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author Beuchert Tobias
Kadler Matthias
Wilms Jörn
Angelakis Emmanouil
Fuhrmann Lars
Myserlis Ioannis
Nestoras Ioannis
Kraus Alex
Bach Uwe
Ros Eduardo
Grossberger Christoph
Schulz Robert
author_facet Beuchert Tobias
Kadler Matthias
Wilms Jörn
Angelakis Emmanouil
Fuhrmann Lars
Myserlis Ioannis
Nestoras Ioannis
Kraus Alex
Bach Uwe
Ros Eduardo
Grossberger Christoph
Schulz Robert
author_sort Beuchert Tobias
collection DOAJ
description Studying the variability of polarized AGN jet emission in the radio band is crucial for understanding the dynamics of moving shocks as well as the structure of the underlying magnetic field. The 100-m Effelsberg Telescope is a high-quality instrument for studying the long-term variability of both total and polarized intensity as well as the electric-vector position angle. Since 2007, the F-GAMMA program has been monitoring the linear polarized emission of roughly 60 blazars at 11 frequencies between 2.7 and 43 GHz. Here, we describe the calibration of the polarimetric data at 5 and 10 GHz and the resulting F-GAMMA full-Stokes light curves for the exemplary case of the radio galaxy 3C 111.
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spelling doaj.art-57d9c588a35341e889de72d4ab6e766f2022-12-21T19:30:55ZengEDP SciencesEPJ Web of Conferences2100-014X2013-12-01610600610.1051/epjconf/20136106006Single-Dish Radio Polarimetry in the F-GAMMA Program with the Effelsberg 100-m Radio TelescopeBeuchert TobiasKadler MatthiasWilms JörnAngelakis EmmanouilFuhrmann LarsMyserlis IoannisNestoras IoannisKraus AlexBach UweRos EduardoGrossberger ChristophSchulz RobertStudying the variability of polarized AGN jet emission in the radio band is crucial for understanding the dynamics of moving shocks as well as the structure of the underlying magnetic field. The 100-m Effelsberg Telescope is a high-quality instrument for studying the long-term variability of both total and polarized intensity as well as the electric-vector position angle. Since 2007, the F-GAMMA program has been monitoring the linear polarized emission of roughly 60 blazars at 11 frequencies between 2.7 and 43 GHz. Here, we describe the calibration of the polarimetric data at 5 and 10 GHz and the resulting F-GAMMA full-Stokes light curves for the exemplary case of the radio galaxy 3C 111.http://dx.doi.org/10.1051/epjconf/20136106006
spellingShingle Beuchert Tobias
Kadler Matthias
Wilms Jörn
Angelakis Emmanouil
Fuhrmann Lars
Myserlis Ioannis
Nestoras Ioannis
Kraus Alex
Bach Uwe
Ros Eduardo
Grossberger Christoph
Schulz Robert
Single-Dish Radio Polarimetry in the F-GAMMA Program with the Effelsberg 100-m Radio Telescope
EPJ Web of Conferences
title Single-Dish Radio Polarimetry in the F-GAMMA Program with the Effelsberg 100-m Radio Telescope
title_full Single-Dish Radio Polarimetry in the F-GAMMA Program with the Effelsberg 100-m Radio Telescope
title_fullStr Single-Dish Radio Polarimetry in the F-GAMMA Program with the Effelsberg 100-m Radio Telescope
title_full_unstemmed Single-Dish Radio Polarimetry in the F-GAMMA Program with the Effelsberg 100-m Radio Telescope
title_short Single-Dish Radio Polarimetry in the F-GAMMA Program with the Effelsberg 100-m Radio Telescope
title_sort single dish radio polarimetry in the f gamma program with the effelsberg 100 m radio telescope
url http://dx.doi.org/10.1051/epjconf/20136106006
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