Structure of the magnetoionic medium around the Fanaroff-Riley Class I radio galaxy 3C 449

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Table 4:

Normalizations and expected depolarization for the individual CPL, joint CPL and joint BPL fit parameters at 1.25 arcsec.
Region	Observed $\langle k\rangle$	CPL			JOINT CPL		JOINT BPL
		C₀	$f_{\rm max}$	$\langle k\rangle$	C₀	$\langle k\rangle$	D₀	$\langle k\rangle$
	(rad² m^-4)		( $\rm arcsec^{-1}$ )	(rad² m^-4)		(rad² m^-4)		(rad² m^-4)
N LOBE	61 $\pm$ 6	0.96	1.60	63 $\pm$ 3	1.52	66 $\pm$ 3	1.91	52 $\pm$ 4
N JET	106 $\pm$ 12	1.34	1.21	106 $\pm$ 5	4.76	110 $\pm$ 5	0.5	109 $\pm$ 5
S JET	91 $\pm$ 11	1.50	1.95	70 $\pm$ 5	1.94	73 $\pm$ 5	1.52	65 $\pm$ 4
S LOBE	50 $\pm$ 5	1.18	1.68	53 $\pm$ 2	1.28	50 $\pm$ 2	2.20	45 $\pm$ 3

Notes. Column 1: region; Col. 2: observed Burn law $\langle k\rangle$ . Columns 3-5: normalization constant C₀, fitted maximum spatial frequency $f_{\rm max}$ for the best CPL power spectrum of each region and the predicted $\langle k\rangle$ for each power spectrum. Columns 6, 7 as Cols. 3 and 5 but for the joint fit to each CPL power spectrum; Cols. 8 and 9 as Cols. 3, and 5 but for the joint BPL power spectrum. For both the joint CPL and BPL fits, the maximum frequency is fixed at $f_{\rm max}= 1.67~{\rm arcsec}^{-1}$ . In calculating each value of $\langle k\rangle$ only data with $p>4\sigma_p$ are included.

Source LaTeX | All tables | In the text

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