Table 1:

Jet properties of the blazars in the Metsähovi-MOJAVE sample.

IAU name	Class	z	1					LAT-det.2
(B1950.0)						(deg)	(deg)
0003-066	BL Lac	0.347	0.9	5.1	2.7	4.0	20.5	N
0003-066	Quasar	1.781	6.7	7.8	6.9	7.3	82.0	N
0003-066	Quasar	2.099	26.5	18.2	28.4	2.9	111.0	N
0003-066	BL Lac	0.265	...	9.1	...	...	...	Y
0003-066	Quasar	0.859	13.0	20.5	14.4	2.5	64.8	Y
0003-066	Quasar	0.405	6.4	15.0	8.9	2.8	46.6	N
0003-066	Quasar	2.367	7.6	8.4	7.7	6.8	84.9	N
0003-066	Quasar	1.207	12.3	16.0	12.7	3.5	75.4	Y
0003-066	BL Lac	0.940	...	23.8	...	...	...	Y
0003-066	Quasar	1.259	12.8	22.0	14.7	2.3	60.5	N
0003-066	Quasar	0.852	22.4	17.2	23.2	3.2	104.9	N
0003-066	Quasar	0.915	7.3	19.7	11.3	1.9	41.0	Y
0003-066	Quasar	2.286	16.5	15.7	16.6	3.7	93.1	N
0003-066	Quasar	2.070	19.2	30.9	21.4	1.7	63.7	Y
0003-066	Quasar	0.872	16.8	7.5	22.6	5.7	131.8	N
0003-066	Quasar	3.396	0.8	10.6	5.4	0.8	8.3	N
0003-066	BL Lac	0.310	10.1	10.8	10.2	5.3	86.4	Y
0003-066	Quasar	0.191	14.4	8.5	16.5	5.9	119.0	N
0003-066	BL Lac	0.266	14.4	5.5	21.6	6.9	138.0	N
0003-066	Quasar	1.436	1.8	35.2	17.6	0.2	6.0	N
0003-066	BL Lac	0.245	1.7	4.6	2.7	8.6	42.8	Y
0003-066	Quasar	0.941	22.0	13.0	25.2	3.9	119.0	N
0003-066	Quasar	2.218	25.4	16.1	28.1	3.2	115.2	N
0003-066	BL Lac	0.306	5.2	16.8	9.3	1.9	34.5	Y
0003-066	Quasar	0.695	0.6	4.3	2.3	3.9	16.7	N
0003-066	Quasar	1.249	18.6	6.3	30.5	5.5	142.4	N
0003-066	Quasar	0.888	8.1	12.1	8.8	4.4	67.6	Y
0003-066	Quasar	0.729	24.9	28.2	25.1	2.0	82.9	Y
0003-066	Quasar	0.432	21.0	5.2	45.5	5.1	152.5	N
0003-066	Quasar	0.158	13.4	16.8	13.8	3.3	77.1	Y
0003-066	Quasar	0.536	20.6	23.8	20.8	2.4	81.9	Y
0003-066	Quasar	0.997	20.9	15.3	22.0	3.6	107.8	Y
0003-066	Quasar	1.400	...	21.0	...	...	...	N
0003-066	Quasar	0.539	10.3	8.3	10.6	6.8	102.6	N
0003-066	BL Lac	0.247	1.8	12.1	6.2	1.4	17.1	N
0003-066	Quasar	1.839	14.8	11.9	15.2	4.7	102.6	Y
0003-066	Quasar	0.360	20.2	16.5	20.6	3.4	101.4	Y
0003-066	BL Lac	0.605	8.7	4.3	11.2	10.6	128.5	N
0003-066	Quasar	1.226	17.9	24.8	18.9	2.2	71.8	N
0003-066	Quasar	1.397	5.7	13.6	8.0	3.0	45.9	N
0003-066	Quasar	1.814	29.5	21.3	31.1	2.6	108.4	Y
0003-066	Quasar	0.751	10.6	13.9	11.0	4.0	75.0	N
0003-066	Quasar	0.593	19.3	7.7	28.0	5.1	136.4	N
0003-066	Quasar	0.902	35.7	10.6	65.5	2.9	146.9	N
0003-066	Quasar	1.379	...	26.3	...	...	...	N
0003-066	Quasar	1.054	...	19.5	...	...	...	N
0003-066	BL Lac	0.322	6.8	11.9	8.0	4.2	60.1	Y
0003-066	BL Lac	0.684	9.0	12.1	9.4	4.5	73.4	Y
0003-066	BL Lac	0.051	0.1	1.1	1.0	45.3	50.8	N
0003-066	BL Lac	0.664	9.4	6.3	10.2	8.4	112.4	N
0003-066	Quasar	0.692	13.7	5.6	19.5	7.1	135.4	N
0003-066	Quasar	0.302	7.2	1.9	15.0	14.8	151.2	N
0003-066	Quasar	1.941	8.4	15.2	9.9	3.2	58.1	N
0003-066	Quasar	1.932	2.0	16.0	8.1	0.9	14.6	N
0003-066	Quasar	2.427	3.0	8.2	4.7	4.5	39.9	N
0003-066	Quasar	0.990	2.2	15.5	7.9	1.0	16.2	N
0003-066	BL Lac	0.069	5.0	7.2	5.4	7.5	69.7	Y
0003-066	Quasar	0.295	7.9	6.6	8.1	8.5	100.3	N
0003-066	Quasar	1.404	14.6	15.9	14.7	3.6	85.4	N
0003-066	Quasar	1.562	8.1	15.8	10.0	3.0	54.8	Y
0003-066	Quasar	1.037	15.4	15.5	15.4	3.7	89.9	Y
0003-066	Quasar	0.859	14.2	32.9	19.5	1.3	46.7	Y

Notes. ⁽¹⁾ Fastest non-accelerating, radial apparent speed measured in the source. The speeds differ in some cases from the speeds quoted by Hovatta et al. (2009), partly because Hovatta et al. used results from a preliminary kinematics analysis, and partly because we consider only non-accelerating, radially moving components in order to estimate the flow speed close to the core, where the mm-wavelength outbursts take place. Due to this, the values of and naturally also differ in some cases from those reported by Hovatta et al. ⁽²⁾ Bright ( ) LAT-detections during the first three months of science operations (Abdo et al. 2009a).