Table 1: Parameters of the FR 1 galaxies, derived in the same way as by Haas et al. (2004). $L_{\rm eml}=L$ (H $_\alpha$ +[NII]) is adopted from Zirbel & Baum (1995).
3CR D_L $L_{\rm MIR}$ $L_{\rm FIR}$ $P_{\rm 15~\mu m}$ $P_{\rm 178~MHz}$ $T_{\rm dust}$ $M_{\rm dust}$ $L_{\rm eml}$

Mpc log [ $L_{\odot}$ ] log [ $L_{\odot}$ ] log [W] log [W] [K] log [ $M_{\odot}$ ] log [W]

31.0 70 <9.23 <9.84 <35.55 33.25 $\sim$ 24 $\sim$ 7.00 ...

66 B 91 <8.85 <9.47 <35.10 33.64 $\sim$ 29 $\sim$ 6.23 ...

76.1 136 <9.21 <9.97 <35.35 33.70 $\sim$ 28 $\sim$ 6.82 ...

84.0 74 0.87 10.80 37.11 33.85 35 7.01 34.91

270.0 31 8.84 9.05 35.10 33.03 28 5.81 32.76

272.1 12 8.13 8.33 34.46 31.90 27 5.13 32.37

274.0 16 8.43 8.50 34.72 32.56 35 4.75 33.47

293.0 197 9.98 10.43 36.32 34.04 26 7.41 34.55

296.0 104 <9.24 <9.64 <35.57 33.45 $\sim$ 27 $\sim$ 6.51 ...

305.0 179 9.97 10.23 36.29 34.04 32 6.66 33.12

338.0 123 9.29 <10.02 35.52 34.21 27 6.95 33.77

**Table 1:** Parameters of the FR 1 galaxies, derived in the same way as by Haas et al. (2004). $L_{\rm eml}=L$ (H $_\alpha$ +[NII]) is adopted from Zirbel & Baum (1995).
3CR	D_L	$L_{\rm MIR}$	$L_{\rm FIR}$	$P_{\rm 15~\mu m}$	$P_{\rm 178~MHz}$	$T_{\rm dust}$	$M_{\rm dust}$	$L_{\rm eml}$
	Mpc	log [ $L_{\odot}$ ]	log [ $L_{\odot}$ ]	log [W]	log [W]	[K]	log [ $M_{\odot}$ ]	log [W]
31.0	70	<9.23	<9.84	<35.55	33.25	$\sim$ 24	$\sim$ 7.00	...
66 B	91	<8.85	<9.47	<35.10	33.64	$\sim$ 29	$\sim$ 6.23	...
76.1	136	<9.21	<9.97	<35.35	33.70	$\sim$ 28	$\sim$ 6.82	...
84.0	74	0.87	10.80	37.11	33.85	35	7.01	34.91
270.0	31	8.84	9.05	35.10	33.03	28	5.81	32.76
272.1	12	8.13	8.33	34.46	31.90	27	5.13	32.37
274.0	16	8.43	8.50	34.72	32.56	35	4.75	33.47
293.0	197	9.98	10.43	36.32	34.04	26	7.41	34.55
296.0	104	<9.24	<9.64	<35.57	33.45	$\sim$ 27	$\sim$ 6.51	...
305.0	179	9.97	10.23	36.29	34.04	32	6.66	33.12
338.0	123	9.29	<10.02	35.52	34.21	27	6.95	33.77

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