(Appendix B, Figures) Polarization flare of 3C 454.3 in millimeter wavelengths seen from decadal polarimetric observations

The B.1. Figures describe the observational results from the KVN single-dish showing flux density (first column), spectral index (α, second column), polarizationdegree (m_p, third column), observed polarization angle (χ_obs, fourth column), and estimated RM in logarithmic scale (fifth column). The filledand open dots in the first and second columns indicate total and linearly polarized emission, respectively. The indicated RM_fit values in the fourthcolumn are in order of 10^3 rad m^−2. The grey shaded area in the last column indicates the range of |RM_fit|. The red solid lines in the fourth and lastcolumns are the fit models to χ = χ_0 + RM λ^2 and |RM| ∝ ν_a, respectively. The corresponding observing dates are noted in the first column. Theminor ticks in the fourth column indicate 5 degree variation The B.2. Figure shows absolute RM values from the KVN observations containing at least two frequency pairs. The grey shaded area is the same as inFigure B.1.

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Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2025-02-27
DOI
https://doi.org/10.5281/zenodo.14967588
Primary Topic
Solar and Space Plasma Dynamics
Type
article
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article

(Appendix B, Figures) Polarization flare of 3C 454.3 in millimeter wavelengths seen from decadal polarimetric observations

Zenodo (CERN European Organization for Nuclear Research)
Solar and Space Plasma Dynamics
article

(Appendix B, Figures) Polarization flare of 3C 454.3 in millimeter wavelengths seen from decadal polarimetric observations

article en

Abstract

The B.1. Figures describe the observational results from the KVN single-dish showing flux density (first column), spectral index (α, second column), polarizationdegree (m_p, third column), observed polarization angle (χ_obs, fourth column), and estimated RM in logarithmic scale (fifth column). The filledand open dots in the first and second columns indicate total and linearly polarized emission, respectively. The indicated RM_fit values in the fourthcolumn are in order of 10^3 rad m^−2. The grey shaded area in the last column indicates the range of |RM_fit|. The red solid lines in the fourth and lastcolumns are the fit models to χ = χ_0 + RM λ^2 and |RM| ∝ ν_a, respectively. The corresponding observing dates are noted in the first column. Theminor ticks in the fourth column indicate 5 degree variation The B.2. Figure shows absolute RM values from the KVN observations containing at least two frequency pairs. The grey shaded area is the same as inFigure B.1.

Zenodo (CERN European Organization for Nuclear Research)
Institute of Astronomy and Astrophysics, Academia Sinica (TW), Seoul National University (KR), Korea Astronomy and Space Science Institute (KR), Astronomy and Space (AU), Korea University of Science and Technology (KR)
Openalex Percentile: Top 63%
Solar and Space Plasma Dynamics
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