Table 8:

CJF sources observed to have a companion and sources showing evidence of an ongoing interaction with another system.

Source	Other name	Type	z	m	Cluster	Companion	Separation	Interaction
				(mag)			(kpc)
0018+729		G	0.821					91
0108+388	OC 314	G	0.669	22				91
0316+413	3C 84	G	0.018	11.9	67	92	600	92
0402+379	4C 37.11	G	0.055	18.5		2	29	2
0710+439		G	0.518	20.4	62	93*	53	93
0804+499	OJ508	Q	1.432	17.5				97
0831+557	4C 55.16	G	0.240	17.5	74	93*	81	93*
0954+658		BL	0.368	16.7		94	474
1031+567	COINS J1035+5628	G	0.460	20.2	91	80	65	49
1146+596	NGC3894	G	0.011	13	84			98
1254+571	Mrk 231	G	0.042	13.6	85	37	361	37
1418+546	OQ530	BL	0.151	15.5	82			99
1641+399	3C345	Q	0.595	16	88	22,95	47
1652+398	Mkn 501	BL	0.034	13.8	89			99
1807+698	3C 371.0	BL	0.051	14.8	82	94	81	99
1823+568	4C 56.27	BL	0.664	18.4		61	46	61
1843+356	COINS J1845+3541	G	0.764	21.9		80*	129	91
1946+708		G	0.101	16.1		96	67	96
2021+614	OW 637	Q	0.227	19	80*	80*	36
2352+495	OZ 488	G	0.237	19	80	80*	47

Notes. 91. Stanghellini et al. (1993); 93. Hutchings et al. (1988); 94. Stickel et al. (1993); 95. Kirhakos et al. (1999); 96. Perlman et al. (2001); 97. Hutchings et al. (1999); 98. Pustilnik et al. (2001); 99. Pursimo et al. (2002).
Columns (1)-(4) as previously, Col. (5) gives the optical magnitude, Col. (6) gives cluster information for comparison (Table 6), Cols. (7) and (8) give references in regard to companion galaxies and their separation respectively, and Col. (9) gives the references in regard to interacting systems. By a star, we indicate ambiguous evidence.