Tracing the merger-driven evolution of active galaxies using the CJF sample

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Table 13:

Variability information and, if available, timescales concerning CJF sources already considered to be BBH candidates.
Source	Type	z	Var ${_{\rm Radio}}$	Var ${_{\rm IR}}$	Var ${_{\rm Opt}}$	Var ${_{\rm X}}$	Var ${_{\gamma}}$
			(yr)		(yr)	(days)	(days)
0316+413	G	0.018	9.7
0402+379	G	0.055	yes
0716+714	BL	0.3	5.4-15	yes	3.3		yes
1101+384	BL	0.0308	3.7-8.0	yes	6.2	62
1641+399	Q	0.595	5.1, 3.5-4	yes	5.6, 11.4, 10.1, 1.9
1652+398	BL	0.03366	6.8-12.3	yes	yes	23	23.2
1803+784	BL	0.6797	7.0-11.3		0.003
1928+738	Q	0.302	7.7-8.2		yes
2200+420	BL	0.0686	3.9-7.8	yes	7.8, 0.6, 0.88, 14, 7.7

Notes. Columns (1)-(3) as before, Col. (4) in the radio, Col. (5) in the infrared, Col. (6) in the optical, Col. (7) in the X-rays, and Col. (8) in the $\gamma$ -rays. For references, see previous tables.

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