Table 3: Lobe spectral ages and estimated source expansion velocity; $\nu _{\rm b}$ and $B_{\rm eq}$ are the break frequency and the equipartition magnetic field. When redshift is unknown, LLS is calculated assuming z = 1.00, and the value is given with a leading " $\sim$ ''.
Name $\nu _{\rm b}$ $B_{\rm eq}$ $t_{\rm syn}$ LLS $v_{\rm sep}$

GHz mG $10^{3}\;$ yr pc h^-1 c

0147+400 7.2 6.2 1.2 $\sim$ 325 0.44

0822+394 22.0 3.3 1.8 260 0.24

0840+424 24.0 2.7 2.3 $\sim$ 530 0.38

1242+410 10.0 5.4 1.3 175 0.22

1432+428 6.5 2.6 4.9 $\sim$ 170 0.06

2330+402 5.3 4.0 2.9 $\sim$ 365 0.21

2358+406 12.0 4.6 1.5 $\sim$ 370 0.40

**Table 3:** Lobe spectral ages and estimated source expansion velocity; $\nu _{\rm b}$ and $B_{\rm eq}$ are the break frequency and the equipartition magnetic field. When redshift is unknown, *LLS* is calculated assuming z = 1.00, and the value is given with a leading " $\sim$ ''.
Name	$\nu _{\rm b}$	$B_{\rm eq}$	$t_{\rm syn}$	LLS	$v_{\rm sep}$
	GHz	mG	$10^{3}\;$ yr	pc	h^-1 c
0147+400	7.2	6.2	1.2	$\sim$ 325	0.44
0822+394	22.0	3.3	1.8	260	0.24
0840+424	24.0	2.7	2.3	$\sim$ 530	0.38
1242+410	10.0	5.4	1.3	175	0.22
1432+428	6.5	2.6	4.9	$\sim$ 170	0.06
2330+402	5.3	4.0	2.9	$\sim$ 365	0.21
2358+406	12.0	4.6	1.5	$\sim$ 370	0.40

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