Comparison between $Fermi$ Detected and non-$Fermi$ Detected Superluminal Sources

TL;DR

This study compares superluminal active galactic nuclei detected and not detected by Fermi-LAT, revealing differences in their apparent velocities, Doppler factors, and viewing angles through statistical analysis of multi-wavelength data.

Contribution

It provides a comprehensive statistical comparison between Fermi-detected and non-Fermi-detected superluminal AGNs, highlighting key differences in their relativistic jet properties.

Findings

Fermi-detected sources have higher proper motions and Lorentz factors.

Fermi-detected sources exhibit smaller viewing angles.

No significant difference in co-moving viewing angles.

Abstract

Active galactic nuclei (AGNs) have been attracting research attention due to their special observable properties. Specifically, a majority of AGNs are detected by Fermi-LAT missions, but not by Fermi-LAT, which raises the question of whether any differences exist between the two. To answer this issue, we compile a sample of 291 superluminal AGNs (189 FDSs and 102 non-FDSs) from available multi-wavelength radio, optical, and X-ray (or even $\gamma$-ray) data and Doppler factors and proper motion ($\mu$) (or apparent velocity ($\beta_{\rm{app}}$)); calculated the apparent velocity from their proper motion, Lorentz factor ($\Gamma$), viewing angle ($\phi$) and co-moving viewing angle ($\phi_{co}$) for the sources with available Doppler factor ($\delta$); and performed some statistical analyses for both types. Our study indicated that1. In terms of average values, FDSs have higher proper motions ($\mu$), apparent velocities ($\beta_{\rm app}$), Doppler factor ($\delta$), Lorentz factor ($\Gamma$), and smaller viewing angle ($\phi$). Nevertheless, there is no clear difference in co-moving viewing angles ($\phi_{\rm co}$).

Tables

Table 1. Table 1: Superluminal Sources detected by Fermi-LAT

FGL name	Class	redshift	${\delta }_R$	Ref	$m_o$	Ext	SR	SX	${\Gamma }_{\gamma }$	F$\gamma$	$\mu$	comp	Ref	$\beta$
Other name					$magnitude$		$mJy$	$1\times {10}^{-12}cgs$		$ph/c{m}^2/s$	$\mu as/yr$
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)	(10)	(11)	(12)	(13)	(14)	(15)
0007+106	G	0.089	2.51	L18	15.8	0.227	98	6.14			204 $\pm$ 12	1	MOJAVE	1.197$\pm$0.069
III ZW 2											269 $\pm$ 50	4	MOJAVE	1.58$\pm$0.29
1FGL J1159.4-2149	F	0.927			17.8	0.104	386	0			9.3 $\pm$ 3.8	1	MOJAVE	0.46$\pm$0.19
1157-215											83 $\pm$ 22	2	MOJAVE	4.1$\pm$1.1
											26.2 $\pm$ 8.0	3	MOJAVE	1.30$\pm$0.40
1FGL J1245.8-0632	F	1.286			19.6	0.068	551	0			358 $\pm$ 53	1	MOJAVE	22.5$\pm$3.4
1243-072											17.6 $\pm$ 8.9e	3	MOJAVE	1.11$\pm$0.56
											40 $\pm$ 16	4	MOJAVE	2.51$\pm$1.00
2FGLJ2148.2+0659	F	0.999	15.6	H09	15.9	0.186	2590	1.46	2.77	3.90E-10	59.0 $\pm$ 1.8	2a	MOJAVE	3.092$\pm$0.096
2145+067											50.1 $\pm$ 9.1	3a	MOJAVE	2.63$\pm$0.48
											49.2 $\pm$ 3.3	5	MOJAVE	2.58$\pm$0.17
											59.3 $\pm$ 3.8	7	MOJAVE	3.11$\pm$0.20
											27.6 $\pm$ 3.8	8	MOJAVE	1.45$\pm$0.20
3FGL J0006.4+3825	F	0.229			17.6	0.205	572	0.75	2.617	6.06E-10	9$\pm$38	C1	CJF	0.12$\pm$0.52
0003+380											135$\pm$37	C2	CJF	1.85$\pm$0.51
											145	C3	CJF	1.99$\pm$0
											336	C4	CJF	4.6$\pm$0

Table 2. Table 2: Superluminal Sources not detected by Fermi-LAT

FGL name	Class	redshift	${\delta }_R$	Ref	$m_o$	Ext	SR	SX	$\mu$	comp	Ref	$\beta$
Other name					$magnitude$		$mJy$	$1\times {10}^{-12}cgs$	$\mu as/yr$
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)	(10)	(11)	(12)	(13)
0003-066	B	0.347	5.1	H09	17.9	0.087	2051	0.82	191 $\pm$ 15	2	MOJAVE	4.09$\pm$0.33
									250 $\pm$ 39	3	MOJAVE	5.36$\pm$0.83
									50.4 $\pm$ 5.3	4a	MOJAVE	1.08$\pm$0.11
									100 $\pm$ 16	5	MOJAVE	2.15$\pm$0.35
									54 $\pm$ 11	6a	MOJAVE	1.16$\pm$0.24
									330.4 $\pm$ 9.8	8a	MOJAVE	7.08$\pm$0.21
									287 $\pm$ 25	9	MOJAVE	6.14$\pm$0.53
									116 $\pm$ 23	14	MOJAVE	2.48$\pm$0.50
0010+405	F	0.255							428 $\pm$ 40	1	MOJAVE	6.92$\pm$0.64
									2 $\pm$ 16e	2	MOJAVE	0.04$\pm$0.26
									2.9 $\pm$ 4.3e	3	MOJAVE	0.047$\pm$0.070
									1.1 $\pm$ 3.1e	4	MOJAVE	0.018$\pm$0.050
0014+813	F	3.366			15.9	0.425	693	0.77	4$\pm$12	C1	B08	0.39$\pm$1.18
									86$\pm$15	C2	B08	8.49$\pm$1.48
									111$\pm$18	C3	B08	10.95$\pm$1.78
0016+731	F	1.781	7.9	H09	18.2	0.735	1136	0.11	106.2 $\pm$ 4.4	1a	MOJAVE	8.23$\pm$0.34
0022+390	F	1.946							113$\pm$43	C1	B08	8.51$\pm$3.24
									71$\pm$57	C2	B08	5.35$\pm$4.29

Table 3. Table 3: Flux density-Flux density correlation analysis results

Type	band	Sample	$a+\Delta a$	$b+\Delta b$	$N$	$r$	$p$
		whole	$0.28\pm 0.04$	$6.15\pm 0.49$	186	0.51	$5.9\times {10}^{-14}$
	$\log S_{r}vs\log F_o$	BL Lac	$0.19\pm 0.06$	$5.08\pm 0.70$	36	0.49	$2.5\times {10}^{-3}$
		FSRQ	$0.34\pm 0.05$	$7.00\pm 0.64$	144	0.49	$3.3\times {10}^{-10}$
		whole	$0.46\pm 0.04$	$5.46\pm 0.51$	180	0.64	$6.8\times {10}^{-22}$
FDS	$\log F_{X}vs\log F_o$	BL Lac	$0.45\pm 0.10$	$5.51\pm 1.19$	36	0.61	$6.7\times {10}^{-5}$
		FSRQ	$0.41\pm 0.05$	$4.87\pm 0.60$	139	0.59	$1.4\times {10}^{-14}$
		whole	$0.53\pm 0.08$	$-1.65\pm 0.22$	179	0.46	$1.0\times {10}^{-10}$
	$\log F_{X}vs\log S_r$	BL Lac	$0.58\pm 0.34$	$-1.51\pm 0.95$	35	0.29	$9.4\%$
		FSRQ	$0.52\pm 0.07$	$-1.72\pm 0.20$	138	0.52	$3.9\times {10}^{-11}$
	$\log S_{r}vs\log F_o$	whole	$0.28\pm 0.07$	$6.21\pm 0.82$	82	0.38	$4.0\times {10}^{-4}$
		FSRQ	$0.28\pm 0.07$	$6.22\pm 0.86$	77	0.43	$1.0\times {10}^{-4}$
non-FDS	$\log F_{X}vs\log F_o$	whole	$0.40\pm 0.06$	$4.63\pm 0.78$	76	0.47	$1.8\times {10}^{-5}$
		FSRQ	$0.36\pm 0.07$	$4.22\pm 0.85$	71	0.54	$1.2\times {10}^{-6}$
	$\log F_{X}vs\log S_r$	whole	$0.51\pm 0.11$	$-1.70\pm 0.30$	76	0.50	$3.7\times {10}^{-6}$
		FSRQ	$0.51\pm 0.11$	$-1.68\pm 0.30$	71	0.49	$1.5\times {10}^{-5}$

Table 4. Table 4: Full table of Table 1

FGL name	Class	redshift	${\delta }_R$	Ref	$m_o$	Ext	SR	SX	${\Gamma }_{\gamma }$	F$\gamma$	$\mu$	comp	Ref	$\beta$
Other name					$magnitude$		$mJy$	$1\times {10}^{-12}cgs$		$ph/c{m}^2/s$	$\mu as/yr$
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)	(10)	(11)	(12)	(13)	(14)	(15)
0007+106	G	0.089	2.51	L18	15.8	0.227	98	6.14			204 $\pm$ 12	1	MOJAVE	1.197$\pm$0.069
III ZW 2											269 $\pm$ 50	4	MOJAVE	1.58$\pm$0.29
1FGL J1159.4-2149	F	0.927			17.8	0.104	386	0			9.3 $\pm$ 3.8	1	MOJAVE	0.46$\pm$0.19
1157-215											83 $\pm$ 22	2	MOJAVE	4.1$\pm$1.1
											26.2 $\pm$ 8.0	3	MOJAVE	1.30$\pm$0.40
1FGL J1245.8-0632	F	1.286			19.6	0.068	551	0			358 $\pm$ 53	1	MOJAVE	22.5$\pm$3.4
1243-072											17.6 $\pm$ 8.9	3	MOJAVE	1.11$\pm$0.56
											40 $\pm$ 16	4	MOJAVE	2.51$\pm$1.00
2FGLJ2148.2+0659	F	0.999	1.2	L18	15.9	0.186	2590	1.46	2.77	3.90E-10	59.0 $\pm$ 1.8	2a	MOJAVE	3.092$\pm$0.096
2145+067											50.1 $\pm$ 9.1	3a	MOJAVE	2.63$\pm$0.48
											49.2 $\pm$ 3.3	5	MOJAVE	2.58$\pm$0.17
											59.3 $\pm$ 3.8	7	MOJAVE	3.11$\pm$0.20
											27.6 $\pm$ 3.8	8	MOJAVE	1.45$\pm$0.20
3FGL J0006.4+3825	F	0.229	5.23	L18	17.6	0.205	572	0.75	2.617	6.06E-10	9$\pm$38	C1	CJF	0.12$\pm$0.52
S4 0003+38											135$\pm$37	C2	CJF	1.85$\pm$0.51
											145	C3	CJF	1.99$\pm$0
											336	C4	CJF	4.6$\pm$0
3FGL J0051.0-0649	F	1.975	5.61	L18	19.5	0.132	905	0.27	2.105	1.40E-09	162 $\pm$ 119	1	MOJAVE	13.4$\pm$9.8
0048-071											131 $\pm$ 10	2	MOJAVE	10.79$\pm$0.85
											20 $\pm$ 23	3	MOJAVE	1.6$\pm$1.9
3FGL J0102.8+5825	F	0.644	18.51	L18	19	11.267	849	0.79	2.094	6.18E-09	140.7 $\pm$ 9.1	2a	MOJAVE	5.20$\pm$0.34
0059+581											185 $\pm$ 13	3a	MOJAVE	6.83$\pm$0.48
											154 $\pm$ 11	4	MOJAVE	5.68$\pm$0.40
											233.2 $\pm$ 8.6	5a	MOJAVE	8.62$\pm$0.32
3FGL J0108.7+0134	F	2.099	2.64	L18	18.1	0.055	2621	0.22	2.26	5.27E-09	139 $\pm$ 14	1a	MOJAVE	11.9$\pm$1.2
0106+013											303 $\pm$ 33	2	MOJAVE	25.8$\pm$2.8
											189.8 $\pm$ 8.2	3a	MOJAVE	16.17$\pm$0.70
											128 $\pm$ 15	4	MOJAVE	10.9$\pm$1.3
3FGL J0110.2+6806	B	0.29			16.5	2.63	0	0.28	1.991	1.92E-09	357 $\pm$ 69	1	MOJAVE	6.5$\pm$1.3
0106+678											91 $\pm$ 22	2	MOJAVE	1.65$\pm$0.41
											23.2 $\pm$ 9.0	3	MOJAVE	0.42$\pm$0.16
											64.1 $\pm$ 7.9	4	MOJAVE	1.16$\pm$0.14
											10.4 $\pm$ 5.4e	5	MOJAVE	0.189$\pm$0.097
3FGL J0112.8+3207	F	0.603	10.21	L18	16.4	0.13	685	4.38	2.363	3.04E-09	427 $\pm$ 12	1	MOJAVE	14.95$\pm$0.44
0110+318											496 $\pm$ 43	2	MOJAVE	17.3$\pm$1.5
											543 $\pm$ 31	3	MOJAVE	19.0$\pm$1.1
3FGL J0116.0-1134	F	0.67	8.22	L18	17.7	0.067	1785	0.9	2.344	1.20E-09	163 $\pm$ 58	1	MOJAVE	6.2$\pm$2.2
0113-118											449 $\pm$ 46	2	MOJAVE	17.2$\pm$1.7
											396 $\pm$ 46	3	MOJAVE	15.2$\pm$1.7
											71 $\pm$ 49	4	MOJAVE	2.7$\pm$1.9
											59 $\pm$ 10	5	MOJAVE	2.25$\pm$0.40
											9 $\pm$ 18e	6	MOJAVE	0.36$\pm$0.70
											125 $\pm$ 60	12	MOJAVE	4.8$\pm$2.3
3FGL J0118.8-2142	F	1.161			17.6	0.032	447	0.14	2.348	3.00E-09	5 $\pm$ 32	1	MOJAVE	0.3$\pm$1.9
0116-219											27 $\pm$ 15	2	MOJAVE	1.59$\pm$0.89
3FGL J0132.6-1655	F	1.02	12.53	L18	18.6	0.046	830	0.27	2.43	1.92E-09	511 $\pm$ 102	3	MOJAVE	27.2$\pm$5.4
0130-171											522 $\pm$ 54	4	MOJAVE	27.8$\pm$2.9
3FGL J0137.0+4752	F	0.859	12.73	L18	18.1	0.346	1138	1.04	2.146	5.10E-09	14.5 $\pm$ 4.8	1a	MOJAVE	0.68$\pm$0.23
133+476											135 $\pm$ 22	2	MOJAVE	6.3$\pm$1.0
											278 $\pm$ 54	3	MOJAVE	13.0$\pm$2.5
											106.4 $\pm$ 6.9	5a	MOJAVE	4.97$\pm$0.32
											354 $\pm$ 12	11	MOJAVE	16.54$\pm$0.56
											200 $\pm$ 25	12	MOJAVE	9.3$\pm$1.2
											52.9 $\pm$ 6.2	13	MOJAVE	2.47$\pm$0.29
3FGL J0145.1-2732	F	1.155			17.5	0.034	923	0.5	2.57	1.36E-09	19 $\pm$ 15	3	MOJAVE	1.09$\pm$0.88
0142-278
3FGL J0204.8+3212	F	1.466	3.08	L18	17.9	0.135	657	0.5	2.945	3.64E-10	148 $\pm$ 15	1	MOJAVE	10.1$\pm$1.0
B2 0202+31											36 $\pm$ 13	2	MOJAVE	2.47$\pm$0.91
3FGL J0205.0+1510	F	0.405	4.71	L18	22	0.122	4068	0.02	2.53	6.71E-10	35.2 $\pm$ 9.5	1	MOJAVE	0.87$\pm$0.23
0202+149											12 $\pm$ 26e	2	MOJAVE	0.31$\pm$0.63
											644 $\pm$ 31	4	MOJAVE	15.88$\pm$0.75
											568 $\pm$ 53	5	MOJAVE	14.0$\pm$1.3
											358 $\pm$ 23	8	MOJAVE	8.82$\pm$0.58
											100 $\pm$ 16	10	MOJAVE	2.47$\pm$0.40
3FGL J0205.2-1700	F	1.739	3.19	L18	17.4	0.072	1220	0.57	2.759	8.59E-10	257 $\pm$ 56	2	MOJAVE	19.6$\pm$4.3
0202-172											208 $\pm$ 41	3	MOJAVE	15.9$\pm$3.1
											68 $\pm$ 24	4	MOJAVE	5.2$\pm$1.8
3FGL J0211.2+1051	B	0.2	8.41	L18	15.4	0.34	319	3.83	2.011	5.30E-09	164 $\pm$ 243	1	MOJAVE	2.1$\pm$3.1
0208+106											377 $\pm$ 56	2	MOJAVE	4.82$\pm$0.72
											332 $\pm$ 54	3	MOJAVE	4.24$\pm$0.69
3FGL J0217.5+7349	F	2.367	66.21	L18	18.9	1.727	2272	0.54	2.1929	4.04E-09	47$\pm$21	C1	B08	3.94$\pm$1.76
0212+735											176$\pm$78	C2	B08	14.74$\pm$6.53
											36$\pm$63	C3	B08	3.01$\pm$5.27
											24$\pm$183	C4	B08	2.01$\pm$15.32
											47$\pm$59	C5	B08	3.94$\pm$4.94
3FGL J0217.8+0143	F	1.715	39.24	L18	16.2	0.076	751	0.56	2.193	4.04E-09	209 $\pm$ 55	1	MOJAVE	15.8$\pm$4.1
PKS 0215+015											333 $\pm$ 15	2a	MOJAVE	25.3$\pm$1.2
											133 $\pm$ 15	3	MOJAVE	10.0$\pm$1.1
3FGL J0222.6+4301	B	0.444	3.4	L18	14.5	0.193	2303	2.29	1.88	1.93E-08	216$\pm$15	C1	B08	5.43$\pm$0.38
3C 66A											42$\pm$24	C2	B08	1.06$\pm$0.6
											219$\pm$93	C3	B08	5.5$\pm$2.34
											552$\pm$187	C4	B08	13.87$\pm$4.7
3FGL J0230.8+4032	F	1.019	27.02	L18	17.7	0.108	451	1.4	2.549	9.56E-10	15$\pm$12	C1	CJF	0.74$\pm$0.59
B3 0227+403											75$\pm$20	C2	CJF	3.71$\pm$0.99
											66$\pm$22	C3	CJF	3.26$\pm$1.09
3FGL J0237.9+2848	F	1.206	11.83	L18	18.1	0.349	2197	0.58	2.162	9.75E-09	345 $\pm$ 16	1	MOJAVE	20.72$\pm$0.97
0234+285											197.0 $\pm$ 6.9	3	MOJAVE	11.84$\pm$0.41
											168.2 $\pm$ 6.5	6	MOJAVE	10.11$\pm$0.39
											157 $\pm$ 12	8	MOJAVE	9.46$\pm$0.73
											409 $\pm$ 24	10	MOJAVE	24.6$\pm$1.4
											8 $\pm$ 15e	12	MOJAVE	0.51$\pm$0.88
3FGL J0238.6+1636	B	0.94	43.53	L18	18.5	0.182	1941	1.24	2.057	1.03E-08	510$\pm$140	C1	PBE06	23.75$\pm$6.52
AO 0235+164											180$\pm$30	C2	PBE06	8.38$\pm$1.4
3FGL J0252.8-2218	F	1.427	11.7	O16	19.8	0.068	443	0.37	2.153	5.34E-09	13 $\pm$ 31	2	MOJAVE	0.9$\pm$2.1
0250-225											18.1 $\pm$ 8.1	3	MOJAVE	1.21$\pm$0.54
3FGL J0303.4-2407	B	0.26			15.4	0.051	700	5.78	1.918	5.74E-09	139 $\pm$ 31	2	MOJAVE	2.33$\pm$0.51
0301-243											56 $\pm$ 39	3	MOJAVE	0.93$\pm$0.66
											87 $\pm$ 21	4	MOJAVE	1.45$\pm$0.34
3FGL J0303.6+4716	B	0.475			16.2	0.593	963	0.36	2.284	2.27E-09	464 $\pm$ 12	1a	MOJAVE	12.38$\pm$0.32
0300+470											54 $\pm$ 15	2	MOJAVE	1.44$\pm$0.40
											19.8 $\pm$ 2.5	3a	MOJAVE	0.53$\pm$0.07
3FGL J0325.2+3410	G	0.061			13.1	0.482	614	3.25	2.438	7.38E-10	115 $\pm$ 52	2	MOJAVE	0.46$\pm$0.21
0321+340											2251 $\pm$ 79	3	MOJAVE	9.05$\pm$0.32
											1312 $\pm$ 246	4	MOJAVE	5.28$\pm$0.99
											95 $\pm$ 37	5	MOJAVE	0.38$\pm$0.15
											34 $\pm$ 23	6	MOJAVE	0.139$\pm$0.091
3FGL J0336.5+3210	F	1.259	5.46	L18	16.6	1.667	2677	2.8	2.887	7.54E-10	167 $\pm$ 16	5	MOJAVE	10.4$\pm$1.0
333+321											210.7 $\pm$ 2.5	6	MOJAVE	13.05$\pm$0.16
											187.1 $\pm$ 7.3	7a	MOJAVE	11.59$\pm$0.45
											125.0 $\pm$ 4.0	10a	MOJAVE	7.74$\pm$0.25
											169.5 $\pm$ 5.6	11	MOJAVE	10.50$\pm$0.35
3FGL J0339.5-0146	F	0.852	23.09	L18	17.1	0.211	2424	0.75	2.253	3.36E-09	154 $\pm$ 17	1a	MOJAVE	7.16$\pm$0.78
0336-019											99.5 $\pm$ 7.3	2a	MOJAVE	4.62$\pm$0.34
											21.1 $\pm$ 3.3	3	MOJAVE	0.98$\pm$0.15
											267 $\pm$ 28	4	MOJAVE	12.4$\pm$1.3
											527 $\pm$ 34	5	MOJAVE	24.5$\pm$1.6
											364.9 $\pm$ 9.4	14a	MOJAVE	16.93$\pm$0.44
3FGL J0349.9-2102	F	2.944			19.7	0.177	305	0.4	2.204	1.28E-09	37 $\pm$ 30	1	MOJAVE	3.8$\pm$3.1
0347-211											25.1 $\pm$ 8.7	2	MOJAVE	2.54$\pm$0.88
3FGL J0405.5-1307	F	0.571	6.53	L18	16.6	0.134	4218	0.97	2.346	5.09E-10	612 $\pm$ 13	1	MOJAVE	20.44$\pm$0.44
PKS 0403-13											80 $\pm$ 15	2	MOJAVE	2.67$\pm$0.49
											623 $\pm$ 19	3a	MOJAVE	20.79$\pm$0.62
											494 $\pm$ 36	4	MOJAVE	16.5$\pm$1.2
											4.8 $\pm$ 2.4e	5	MOJAVE	0.161$\pm$0.079
											335 $\pm$ 41	10	MOJAVE	11.2$\pm$1.4
											514 $\pm$ 29	11	MOJAVE	17.16$\pm$0.96
3FGL J0418.5+3813c	SY1	0.049	2.9	H09					2.787	7.34E-10	1733 $\pm$ 46	2	MOJAVE	5.62$\pm$0.15
0415+379											1613 $\pm$ 93	3	MOJAVE	5.24$\pm$0.30
											1710 $\pm$ 66	7	MOJAVE	5.55$\pm$0.22
											1271 $\pm$ 56	9	MOJAVE	4.13$\pm$0.18
											909 $\pm$ 60	10	MOJAVE	2.95$\pm$0.19
											1810 $\pm$ 27	14	MOJAVE	5.874$\pm$0.089
											1463 $\pm$ 96	15	MOJAVE	4.75$\pm$0.31
											1473 $\pm$ 19	26a	MOJAVE	4.780$\pm$0.060
											993 $\pm$ 127	28	MOJAVE	3.22$\pm$0.41
											2510 $\pm$ 95	30	MOJAVE	8.15$\pm$0.31
											1703 $\pm$ 18	32a	MOJAVE	5.526$\pm$0.059
											1464 $\pm$ 17	33a	MOJAVE	4.752$\pm$0.057
											1875 $\pm$ 78	36	MOJAVE	6.08$\pm$0.25
											1346 $\pm$ 32	37a	MOJAVE	4.37$\pm$0.10
											1547 $\pm$ 148	38	MOJAVE	5.02$\pm$0.48
											1329 $\pm$ 16	39a	MOJAVE	4.314$\pm$0.053
											1275 $\pm$ 17	40a	MOJAVE	4.136$\pm$0.055
											855 $\pm$ 22	41	MOJAVE	2.773$\pm$0.072
3FGL J0423.2-0119	F	0.916	5.31	L18	19.3	0.287	677	0.41	2.204	5.59E-09	107.9 $\pm$ 9.7	1a	MOJAVE	5.30$\pm$0.47
0420-014											74 $\pm$ 11	2	MOJAVE	3.63$\pm$0.55
											95.6 $\pm$ 6.7	3	MOJAVE	4.69$\pm$0.33
											48 $\pm$ 11	4	MOJAVE	2.35$\pm$0.52
3FGL J0442.6-0017	F	0.844	12.61	L18	18.2	0.117	1773	1.7	2.496	3.49E-09	340 $\pm$ 230	B	JM01	14.6$\pm$1.29
0440?003
3FGL J0449.0+1121	F	1.207			19.9	1.158	847	0.26	2.233	2.78E-09	77.7 $\pm$ 5.4	2a	MOJAVE	6.72$\pm$0.46
0446+112											75.0 $\pm$ 8.9	3	MOJAVE	6.48$\pm$0.77
3FGL J0453.2-2808	F	2.559			17.9	0.071	2541	0.22	2.63	1.43E-09	169 $\pm$ 222	1	MOJAVE	16$\pm$21
0451-282											82 $\pm$ 84	2	MOJAVE	7.7$\pm$8.0
											64 $\pm$ 108	3	MOJAVE	6$\pm$10
											121.3 $\pm$ 9.8	4	MOJAVE	11.48$\pm$0.93
											30 $\pm$ 17	5	MOJAVE	2.8$\pm$1.6
3FGL J0457.0-2324	F	1.003			17.9	0.105	1727	0.6	2.039	1.80E-08	282 $\pm$ 34	2a	MOJAVE	14.8$\pm$1.8
0454-234
3FGL J0501.2-0157	F	2.286	24.92	L18	17.9	0.169	2264	0.92	2.414	2.32E-09	27.9 $\pm$ 7.3	2	MOJAVE	2.49$\pm$0.65
0458-020											68 $\pm$ 17	3	MOJAVE	6.0$\pm$1.5
3FGL J0530.8+1330	F	2.07	12.35	L18	18.9	1.964	1556	0.8	2.246	3.69E-09	68 $\pm$ 12	1a	MOJAVE	5.7$\pm$1.1
0528+134											204.9 $\pm$ 6.5	2	MOJAVE	17.33$\pm$0.55
											111.7 $\pm$ 6.3	3a	MOJAVE	9.45$\pm$0.53
											108.0 $\pm$ 9.5	7	MOJAVE	9.13$\pm$0.81
											129 $\pm$ 15	8	MOJAVE	10.9$\pm$1.3
3FGL J0532.7+0732	F	1.254	31.03	L18	17.5	0.707	2729	0.31	2.203	5.86E-09	290 $\pm$ 14	1	MOJAVE	17.92$\pm$0.86
0529+075											141 $\pm$ 16	2	MOJAVE	8.74$\pm$0.99
											200 $\pm$ 19	3	MOJAVE	12.4$\pm$1.2
3FGL J0533.2+4822	F	1.162			18.3	0.913	434	0.23	2.386	2.88E-09	338 $\pm$ 51	3	MOJAVE	19.8$\pm$3.0
TXS 0529+483											211.8 $\pm$ 7.1	4a	MOJAVE	12.38$\pm$0.41
											184 $\pm$ 19	5	MOJAVE	10.8$\pm$1.1
											306 $\pm$ 44	9	MOJAVE	17.9$\pm$2.5
3FGL J0540.5-5416	F	0.839	48.01	L18	20.8	0.99	860	0.2	2.628	6.89E-10	154 $\pm$ 56	1	MOJAVE	7.0$\pm$2.6
0539-057											169 $\pm$ 38	2	MOJAVE	7.7$\pm$1.8
											82 $\pm$ 32	3	MOJAVE	3.7$\pm$1.5
											131 $\pm$ 36	4	MOJAVE	6.0$\pm$1.7
											301 $\pm$ 46	5	MOJAVE	13.8$\pm$2.1
											84 $\pm$ 60	6	MOJAVE	3.8$\pm$2.7
3FGL J0608.0-0835	F	0.872	4.19	L18	15.5	1.345	1905	0.24	2.373	2.09E-09	231 $\pm$ 11	2	MOJAVE	10.90$\pm$0.51
0605-085											410 $\pm$ 13	3	MOJAVE	19.35$\pm$0.59
											328.4 $\pm$ 9.4	4	MOJAVE	15.49$\pm$0.44
											25 $\pm$ 11	5	MOJAVE	1.18$\pm$0.52
											11.0 $\pm$ 5.0e	6	MOJAVE	0.52$\pm$0.24
											678 $\pm$ 108	10	MOJAVE	32.0$\pm$5.1
3FGL J0608.1-1522	F	1.094	29.5	L18	20.5	0.826	279	0.15	2.247	1.55E-09	72 $\pm$ 17	1	MOJAVE	4.04$\pm$0.96
0605-153
3FGL J0622.9+3326	BCU				18.3	0.963	240	0.21	2.095	7.03E-09	635 $\pm$ 61	3	MOJAVE	34.8$\pm$3.3
0619+334
3FGL J0629.4-1959	B	0.63			20.1	0.555	677	0.17	2.182	3.36E-09	106 $\pm$ 132	2	MOJAVE	8$\pm$10
0627-199											25 $\pm$ 24	3	MOJAVE	1.9$\pm$1.8
3FGL J0638.6+7324	F	1.85	17.67	L18	18	0.238	903	0.5	2.641	4.34E-10	57	C0	CJF	4.17$\pm$0
S5 0633+73											212$\pm$3	C1	CJF	15.51$\pm$0.22
											272$\pm$13	C2	CJF	19.9$\pm$0.95
											164$\pm$39	C3	CJF	12$\pm$2.85
											189$\pm$45	C4	CJF	13.83$\pm$3.29
											201$\pm$80	C5	CJF	14.7$\pm$5.85
3FGL J0654.4+4514	F	0.933	18.2	L18	19.8	0.239	382	0.8	2.287	2.88E-09	188 $\pm$ 64	1	MOJAVE	9.3$\pm$3.2
0650+453											89 $\pm$ 19	2	MOJAVE	4.42$\pm$0.92
											29 $\pm$ 15	3	MOJAVE	1.44$\pm$0.75
3FGL J0710.5+4732	B	1.292	8.09	L18	13.9	0.185	1019	0.67	2.648	5.07E-10	34 $\pm$ 10	3	MOJAVE	2.14$\pm$0.66
0707+476											132 $\pm$ 15	4	MOJAVE	8.33$\pm$0.92
											119 $\pm$ 11	5	MOJAVE	7.48$\pm$0.72
3FGL J0721.9+7120	B	0.3	31.33	L18	14.1	0.071	727	2.27	1.948	2.20E-08	638 $\pm$ 44	2a	MOJAVE	5.27$\pm$0.36
716+714											450 $\pm$ 53	3	MOJAVE	3.72$\pm$0.44
											594 $\pm$ 19	5a	MOJAVE	4.91$\pm$0.16
											597 $\pm$ 68	6	MOJAVE	4.93$\pm$0.56
											651 $\pm$ 68	7	MOJAVE	5.37$\pm$0.56
											1400 $\pm$ 98	14	MOJAVE	11.56$\pm$0.81
											2258 $\pm$ 65	16	MOJAVE	18.64$\pm$0.53
											1184 $\pm$ 124	17	MOJAVE	9.8$\pm$1.0
											1539 $\pm$ 31	18a	MOJAVE	12.71$\pm$0.25
											741 $\pm$ 48	19	MOJAVE	6.11$\pm$0.40
											580 $\pm$ 66	20	MOJAVE	4.79$\pm$0.54
											737 $\pm$ 89	21	MOJAVE	6.09$\pm$0.74
3FGL J0725.8-0054	BCU	0.128	2.56	L18	16.6	0.17	1399	3.14	2.359	3.90E-10	126 $\pm$ 18	5	MOJAVE	1.04$\pm$0.15
0723-008											113 $\pm$ 11	6	MOJAVE	0.933$\pm$0.090
3FGL J0733.8+5021	F	0.74	3.28	L18	19.1	0.146	770	0.52	2.504	4.34E-10	345 $\pm$ 101	1	MOJAVE	14.0$\pm$4.1
0730+504											381 $\pm$ 16	2	MOJAVE	15.45$\pm$0.64
3FGL J0738.1+1741	B	0.424	3.8	H09	15.5	0.078	2258	0.97	2.006	5.48E-09	54.8 $\pm$ 4.4	1a	MOJAVE	1.49$\pm$0.12
0735+178											95.7 $\pm$ 5.4	2a	MOJAVE	2.60$\pm$0.15
											186 $\pm$ 22	3	MOJAVE	5.05$\pm$0.61
											144 $\pm$ 10	5a	MOJAVE	3.90$\pm$0.28
											180 $\pm$ 17	6a	MOJAVE	4.88$\pm$0.45
											173 $\pm$ 19	8	MOJAVE	4.69$\pm$0.50
											239 $\pm$ 32	14	MOJAVE	6.48$\pm$0.86
3FGL J0739.4+0137	F	0.19	11.44	L18	16	0.313	1964	2.28	2.245	2.73E-09	304 $\pm$ 11	1a	MOJAVE	3.70$\pm$0.14
0736+017											974 $\pm$ 18	4	MOJAVE	11.83$\pm$0.22
											930 $\pm$ 49	5	MOJAVE	11.30$\pm$0.59
											636 $\pm$ 38	6	MOJAVE	7.73$\pm$0.46
											950 $\pm$ 10	7a	MOJAVE	11.54$\pm$0.13
											743 $\pm$ 17	8	MOJAVE	9.03$\pm$0.21
											880 $\pm$ 82	9	MOJAVE	10.69$\pm$1.00
											979 $\pm$ 22	11	MOJAVE	11.90$\pm$0.27
											703 $\pm$ 58	12	MOJAVE	8.54$\pm$0.70
											330 $\pm$ 55	13	MOJAVE	4.01$\pm$0.67
3FGL J0742.6+5444	F	0.72	21.08	L18	17.6	0.097	281	0.38	2.131	4.67E-09	43 $\pm$ 24	2	MOJAVE	1.74$\pm$0.99
0738+548
3FGL J0750.6+1232	F	0.889	3.46	L18	17.3	0.07	1453	1.73	2.411	9.38E-10	304 $\pm$ 12	2a	MOJAVE	14.57$\pm$0.56
0748+126											208.7 $\pm$ 6.7	3a	MOJAVE	10.01$\pm$0.32
											87.2 $\pm$ 7.4	6	MOJAVE	4.18$\pm$0.36
											120 $\pm$ 14	7	MOJAVE	5.75$\pm$0.68
											89 $\pm$ 10	8	MOJAVE	4.26$\pm$0.48
3FGL J0757.0+0956	F	0.266	11.26	L18	15.1	0.05	956	1.18	2.182	1.86E-09	63 $\pm$ 16	1	MOJAVE	1.05$\pm$0.26
0754+100											860 $\pm$ 72	2	MOJAVE	14.4$\pm$1.2
											594 $\pm$ 42	9	MOJAVE	9.95$\pm$0.71
											12 $\pm$ 14e	12	MOJAVE	0.21$\pm$0.23
											298 $\pm$ 24	13a	MOJAVE	4.99$\pm$0.40
3FGL J0805.4+6144	F	3.033	12.23	L18	19.7	0.133	828	0.8	2.748	6.02E-10	22$\pm$ 89	C1	CJF	2.07$\pm$8.39
TXS 0800+618											77$\pm$ 44	C2	CJF	7.26$\pm$4.15
											97$\pm$ 93	C3	CJF	9.15$\pm$8.77
3FGL J0808.2-0751	F	1.837	35.18	L18	17.8	0.323	1595	0.88	1.958	9.67E-09	105 $\pm$ 41	1	MOJAVE	8.3$\pm$3.2
PKS 0805-07											503 $\pm$ 62	2	MOJAVE	39.7$\pm$4.9
											441 $\pm$ 23	3a	MOJAVE	34.8$\pm$1.8
											165 $\pm$ 29	4	MOJAVE	13.1$\pm$2.3
											269 $\pm$ 27	5	MOJAVE	21.3$\pm$2.1
											109 $\pm$ 22	8	MOJAVE	8.6$\pm$1.7
3FGL J0811.3+0146	B	1.148	21.79	L18	19.2	0.074	598	0.25	2.158	2.46E-09	236 $\pm$ 16	1	MOJAVE	13.70$\pm$0.91
0808+019											200 $\pm$ 18	2	MOJAVE	11.6$\pm$1.1
3FGL J0818.2+4223	B	0.53	4.6	H09	18.1	0.146	1091	0.32	2.006	6.33E-09	64.9 $\pm$ 4.1	2a	MOJAVE	1.9$\pm$0.12
S4 0814+42											32.0 $\pm$ 3.6	5a	MOJAVE	0.94$\pm$0.11
											294 $\pm$ 24	6	MOJAVE	8.62$\pm$0.70
3FGL J0824.9+3916	F	1.216	8.97	L18	17.9	0.105	1481	1.06	2.445	4.66E-10	53 $\pm$ 32	4	MOJAVE	3.2$\pm$1.9
0821+394											17 $\pm$ 22	5	MOJAVE	1.0$\pm$1.3
											28 $\pm$ 13	6	MOJAVE	1.72$\pm$0.81
											145 $\pm$ 13	8	MOJAVE	8.74$\pm$0.80
											86 $\pm$ 22	9	MOJAVE	5.2$\pm$1.3
											35 $\pm$ 14	10	MOJAVE	2.09$\pm$0.84
3FGL J0824.9+5551	F	1.421	26.35	L18	18.1	0.144	1449	0.64	2.606	6.60E-10	17	C1	CJF	1.06$\pm$0
0820+560											32$\pm$ 69	C2	CJF	1.99$\pm$4.29
											79	C3	CJF	4.92$\pm$0
3FGL J0826.0+0307	B	0.506	10.23	L18	18.3	0.101	1400	1.57	2.03	5.26E-10	321 $\pm$ 27	6	MOJAVE	9.64$\pm$0.81
PKS 0823+033											403 $\pm$ 15	7a	MOJAVE	12.11$\pm$0.46
											352 $\pm$ 61	8	MOJAVE	10.6$\pm$1.8
											414 $\pm$ 19	9a	MOJAVE	12.41$\pm$0.58
											32.8 $\pm$ 5.8	12	MOJAVE	0.99$\pm$0.17
											175 $\pm$ 45	13	MOJAVE	5.3$\pm$1.3
3FGL J0830.7+2408	F	0.939	31.97	L18	17.1	0.077	739	1.36	2.6269	1.09E-09	203 $\pm$ 29	1	MOJAVE	10.2$\pm$1.5
0827+243											360.4 $\pm$ 7.6	2	MOJAVE	18.07$\pm$0.38
											395 $\pm$ 25	3	MOJAVE	19.8$\pm$1.3
											367 $\pm$ 10	4a	MOJAVE	18.39$\pm$0.51
3FGL J0831.9+0430	B	0.174	5.94	L18	15.4	0.075	1241	0.6	2.097	3.39E-09	313 $\pm$ 18	2	MOJAVE	3.50$\pm$0.20
PKS 0829+046											329 $\pm$ 26	3	MOJAVE	3.68$\pm$0.29
											5.9 $\pm$ 2.3e	4	MOJAVE	0.066$\pm$0.025
											905 $\pm$ 31	5	MOJAVE	10.14$\pm$0.35
											778 $\pm$ 20	6a	MOJAVE	8.71$\pm$0.23
3FGL J0832.6+4914	B	0.548			19.3	0.099	344	0.15	2.363	2.10E-10	340	K7	GPC99	10.26
0828+493
3FGL J0839.5+0102	F	1.123	5.82	L18	18.7	0.108	422	0.49	2.238	5.44E-10	267 $\pm$ 30	3	MOJAVE	15.2$\pm$1.7
0837+012
3FGL J0840.8+1315	S1,2	0.681	3.31	L18	18.2	0.221	2614	0.48	2.468	5.18E-10	264.3 $\pm$ 6.4	1a	MOJAVE	10.22$\pm$0.25
0838+133											246.1 $\pm$ 3.7	2	MOJAVE	9.52$\pm$0.14
											251.0 $\pm$ 6.5	3a	MOJAVE	9.71$\pm$0.25
											289.6 $\pm$ 8.8	5	MOJAVE	11.20$\pm$0.34
											166 $\pm$ 36	6	MOJAVE	6.4$\pm$1.4
											136 $\pm$ 12	11	MOJAVE	5.24$\pm$0.48
											105 $\pm$ 14	14	MOJAVE	4.06$\pm$0.54
3FGL J0841.4+7053	F	2.218	16.3	H09	16.8	0.069	3823	5.52	2.616	1.26E-09	221.9 $\pm$ 8.5	1a	MOJAVE	19.49$\pm$0.75
0836+710											193 $\pm$ 19	2	MOJAVE	17.0$\pm$1.7
											145.3 $\pm$ 9.5	3	MOJAVE	12.76$\pm$0.83
											191.3 $\pm$ 4.7	4a	MOJAVE	16.80$\pm$0.41
											216.3 $\pm$ 7.0	5	MOJAVE	19.00$\pm$0.61
											201.5 $\pm$ 6.8	6	MOJAVE	17.70$\pm$0.60
											240.2 $\pm$ 8.8	7	MOJAVE	21.10$\pm$0.77
3FGL J0854.8+2006	B	0.306	29.77	L18	15.4	0.064	1512	1.79	2.122	5.90E-09	580 $\pm$ 23	1a	MOJAVE	11.08$\pm$0.44
851+202											793 $\pm$ 22	4	MOJAVE	15.14$\pm$0.43
											538.4 $\pm$ 7.0	5a	MOJAVE	10.28$\pm$0.13
											198 $\pm$ 35	9a	MOJAVE	3.78$\pm$0.66
											22.9 $\pm$ 2.0	10a	MOJAVE	0.438$\pm$0.038
											345 $\pm$ 30	11	MOJAVE	6.58$\pm$0.56
											270 $\pm$ 20	15	MOJAVE	5.15$\pm$0.38
3FGL J0903.1+4649	F	1.465			19	0.044	1755	0.25	2.615	2.94E-10	127.1 $\pm$ 9.5	1	MOJAVE	8.70$\pm$0.65
0859+470											235 $\pm$ 19	3	MOJAVE	16.1$\pm$1.3
3FGL J0909.1+0121	F	1.026	38.61	L18	17.4	0.079	760	0.69	2.458	3.80E-09	343 $\pm$ 17	4	MOJAVE	18.33$\pm$0.89
0906+015											366.7 $\pm$ 5.7	5	MOJAVE	19.61$\pm$0.31
											399.5 $\pm$ 5.9	7	MOJAVE	21.36$\pm$0.31
3FGL J0920.9+4442	F	2.189	26.6	L18	17.9	0.048	1017	1.04	2.135	5.78E-09	165 $\pm$ 20	2	MOJAVE	14.4$\pm$1.8
0917+449											7.3 $\pm$ 2.9	3a	MOJAVE	0.64$\pm$0.25
											48 $\pm$ 16	4	MOJAVE	4.2$\pm$1.4
											108 $\pm$ 21	7	MOJAVE	9.5$\pm$1.8
											87.9 $\pm$ 8.0	8	MOJAVE	7.67$\pm$0.70
3FGL J0921.8+6215	F	1.446	22.37	L18	18.7	0.106	946	0	2.448	1.14E-09	200 $\pm$ 27	1	MOJAVE	13.7$\pm$1.9
0917+624											9.7 $\pm$ 3.7e	2	MOJAVE	0.66$\pm$0.26
											136 $\pm$ 10	3	MOJAVE	9.28$\pm$0.70
											134.6 $\pm$ 8.2	5a	MOJAVE	9.18$\pm$0.56
											60.6 $\pm$ 8.7	6a	MOJAVE	4.13$\pm$0.59
											89 $\pm$ 24	10	MOJAVE	6.0$\pm$1.6
											143 $\pm$ 14	11	MOJAVE	9.76$\pm$0.96
3FGL J0940.7-6102	F	0.551			18.4	0.101	290	0	2.409	6.33E-10	37 $\pm$ 53	3	MOJAVE	1.2$\pm$1.7
0938-133
3FGL J0948.6+4041	F	1.249	1.87	L18	17.6	0.031	1600	0.25	2.669	3.03E-10	174 $\pm$ 12	1a	MOJAVE	10.74$\pm$0.71
0945+408											149 $\pm$ 22	2	MOJAVE	9.2$\pm$1.4
											197.2 $\pm$ 6.1	3	MOJAVE	12.15$\pm$0.38
											230.5 $\pm$ 6.6	4a	MOJAVE	14.20$\pm$0.40
											290.4 $\pm$ 7.5	5	MOJAVE	17.89$\pm$0.46
											328 $\pm$ 15	6	MOJAVE	20.21$\pm$0.95
3FGL J0948.8+0021	F	0.585	29.77	L18	18.4	0.18	70	2.99	2.317	2.65E-09	338 $\pm$ 44	2a	MOJAVE	11.5$\pm$1.5
0946+006											161 $\pm$ 57	3	MOJAVE	5.5$\pm$1.9
3FGL J0956.6+2515	F	0.707	8.02	L18	17.9	0.086	1080	0.5	2.436	8.88E-10	164 $\pm$ 16	1	MOJAVE	6.55$\pm$0.63
0953+254											104 $\pm$ 12	3	MOJAVE	4.18$\pm$0.48
											180 $\pm$ 48	4	MOJAVE	7.2$\pm$1.9
											163.9 $\pm$ 3.9	5a	MOJAVE	6.56$\pm$0.16
											251.3 $\pm$ 3.8	6a	MOJAVE	10.05$\pm$0.15
											149 $\pm$ 22	7	MOJAVE	5.95$\pm$0.90
											178.6 $\pm$ 9.7	8	MOJAVE	7.14$\pm$0.39
											106 $\pm$ 18	9	MOJAVE	4.22$\pm$0.73
3FGL J0958.6+6534	B	0.367	6.2	H09	15.5	0.273	729	0.52	2.381	1.38E-09	6 $\pm$ 19e	2	MOJAVE	0.13$\pm$0.40
0954+658											499 $\pm$ 23	9a	MOJAVE	10.58$\pm$0.49
											271 $\pm$ 24	10	MOJAVE	5.75$\pm$0.51
											346 $\pm$ 20	11	MOJAVE	7.34$\pm$0.42
											467 $\pm$ 53	12	MOJAVE	9.91$\pm$1.12
											290 $\pm$ 35	13	MOJAVE	6.15$\pm$0.74
											672 $\pm$ 52	14	MOJAVE	14.25$\pm$1.10
											270 $\pm$ 11	18	MOJAVE	5.73$\pm$0.23
3FGL J1015.0+4925	B	0.212	0.44	L18	15.5	0.027	378	13.2	1.83	7.35E-09	152 $\pm$ 63	2	MOJAVE	2.06$\pm$0.85
1ES 1011+496											131 $\pm$ 27	3	MOJAVE	1.78$\pm$0.37
											24 $\pm$ 35	4	MOJAVE	0.33$\pm$0.47
											44 $\pm$ 23	5	MOJAVE	0.59$\pm$0.31
3FGL J1018.3+3542	F	1.23	12.5	L18	17.9	0.027	616	0.26	2.549	2.75E-10	136.0 $\pm$ 9.5	1	MOJAVE	8.28$\pm$0.58
1015+359											139 $\pm$ 14	2	MOJAVE	8.47$\pm$0.82
											62 $\pm$ 11	3	MOJAVE	3.79$\pm$0.64
											452 $\pm$ 64	10	MOJAVE	27.5$\pm$3.9
											214 $\pm$ 29	11	MOJAVE	13.0$\pm$1.8
3FGL J1023.1+3952	F	1.254	12.06	L18	18	0.03	1123	0.47	2.726	2.88E-10	28$\pm$52	C1	CJF	1.6$\pm$2.98
1020+400											211$\pm$58	C2	CJF	12.08$\pm$3.32
											212$\pm$82	C3	CJF	12.14$\pm$4.7
3FGL J1033.2+4116	F	1.12	9.59	L18	19.1	0.029	474	0.57	2.3217	1.27E-09	41$\pm$81	C1	CJF	2.36$\pm$4.67
1030+415											73$\pm$42	C2	CJF	4.21$\pm$2.42
											17	C3	CJF	0.98
3FGL J1033.8+6051	F	1.409	41.41	L18	18.5	0.023	462	0.91	2.119	5.24E-09	200 $\pm$ 49	3	MOJAVE	13.3$\pm$3.3
1030+611											97.4 $\pm$ 5.6	4a	MOJAVE	6.49$\pm$0.37
3FGL J1040.4+0615	F	1.264	13.88	L18	16.9	0.056	1406	1.71	2.52	1.44E-09	55.3 $\pm$ 9.9	1	MOJAVE	3.44$\pm$0.61
1038+064											80.8 $\pm$ 5.5	3	MOJAVE	5.02$\pm$0.34
											147.5 $\pm$ 9.5	4	MOJAVE	9.17$\pm$0.59
											55.9 $\pm$ 8.0	5	MOJAVE	3.47$\pm$0.50
											158 $\pm$ 13	6	MOJAVE	9.85$\pm$0.82
3FGL J1044.4+8058	F	1.26	13.78	L18	17.9	0.056	828	0.74	2.76	3.08E-10	38$\pm$54	C1	CJF	2.18$\pm$3.1
S5 1039+81											163$\pm$25	C2	CJF	9.36$\pm$1.44
											45$\pm$98	C3	CJF	2.59$\pm$5.63
											143$\pm$376	C4	CJF	8.21$\pm$21.6
3FGL J1048.4+7144	F	1.15	30.71	L18	17.5	0.144	737	0.88	2.392	2.79E-09	64 $\pm$ 17	2a	MOJAVE	3.71$\pm$0.98
1044+719
3FGL J1058.5+0133	B	0.89	34.9	L18	17.9	0.06	3220	1.08	2.171	6.51E-09	76 $\pm$ 38	2	MOJAVE	3.6$\pm$1.8
1055+018											146 $\pm$ 14	3	MOJAVE	6.98$\pm$0.68
											27.2 $\pm$ 5.4	4	MOJAVE	1.30$\pm$0.26
											4.2 $\pm$ 2.0e	5	MOJAVE	0.199$\pm$0.096
3FGL J1058.6+5627	B	0.143243	0.38	L18	16	0.027	229	3.13	1.945	3.63E-09	123 $\pm$ 34	1	MOJAVE	1.14$\pm$0.31
1055+567											10.0 $\pm$ 6.1e	2	MOJAVE	0.092$\pm$0.056
3FGL J1104.4+3812	B	0.03	2.03	L18	13.1	0.035	767	180	1.772	3.03E-08	1330$\pm$20	C1	VC94	2.51$\pm$0.04
1101+384											940$\pm$150	C2	VC94	1.77$\pm$0.28
3FGL J1121.4-0554	F	1.297	8.97	L18	17.6	0.084	588	0.35	2.366	2.22E-09	46 $\pm$ 103	1	MOJAVE	2.9$\pm$6.5
1118-056											17 $\pm$ 14	3	MOJAVE	1.04$\pm$0.91
											23 $\pm$ 24	4	MOJAVE	1.4$\pm$1.5
3FGL J1129.9-1446	F	1.184	12.1	L18	16	0.083	5622	1.39	2.787	8.95E-10	195.3 $\pm$ 5.3	2a	MOJAVE	11.59$\pm$0.31
PKS 1127-14											31.2 $\pm$ 2.4	3a	MOJAVE	1.85$\pm$0.14
											218.4 $\pm$ 9.5	4a	MOJAVE	12.96$\pm$0.56
											54.7 $\pm$ 8.1	5a	MOJAVE	3.25$\pm$0.48
											265.5 $\pm$ 7.7	8	MOJAVE	15.75$\pm$0.46
											126 $\pm$ 16	12	MOJAVE	7.49$\pm$0.97
											319 $\pm$ 68	13	MOJAVE	18.9$\pm$4.0
3FGL J1146.8+3958	F	1.09	29.39	L18	18.3	0.04	331	0.69	2.231	3.34E-09	23 $\pm$ 13	3	MOJAVE	1.28$\pm$0.70
1144+402
3FGL J1147.8-0725	F	1.342	15.11	L18	18.3	0.089	740	0.34	2.317	1.39E-09	192.3 $\pm$ 7.2	3	MOJAVE	12.44$\pm$0.47
1145-071											211 $\pm$ 42	4	MOJAVE	13.6$\pm$2.7
3FGL J1159.5+2914	F	0.725	32.92	L18	18.1	0.045	2031	0.84	2.095	8.37E-09	43.3 $\pm$ 6.6	2	MOJAVE	1.77$\pm$0.27
1156+295											302 $\pm$ 36	4	MOJAVE	12.3$\pm$1.5
											603 $\pm$ 48	7	MOJAVE	24.6$\pm$1.9
											517 $\pm$ 48	8	MOJAVE	21.1$\pm$1.9
											516 $\pm$ 47	9	MOJAVE	21.0$\pm$1.9
3FGL J1205.8-2636	F	0.789			19.3	0.19	1654	0.63	2.541	7.58E-10	245 $\pm$ 76	2	MOJAVE	10.7$\pm$3.3
1202-262											102 $\pm$ 23	3	MOJAVE	4.46$\pm$0.99
3FGL J1221.4+2814	B	0.102	2.67	L18	15	0.053	732	1.3	2.102	4.12E-09	545 $\pm$ 39	1	MOJAVE	3.67$\pm$0.26
1219+285											1356 $\pm$ 118	4	MOJAVE	9.12$\pm$0.80
											1061 $\pm$ 108	7	MOJAVE	7.14$\pm$0.73
											885 $\pm$ 35	8	MOJAVE	5.96$\pm$0.23
											766 $\pm$ 58	9a	MOJAVE	5.16$\pm$0.39
											894 $\pm$ 117	10	MOJAVE	6.02$\pm$0.79
											83.3 $\pm$ 7.9	12	MOJAVE	0.561$\pm$0.053
											514 $\pm$ 15	15a	MOJAVE	3.460$\pm$0.099
											18.7 $\pm$ 3.7e	17	MOJAVE	0.126$\pm$0.025
											3.2 $\pm$ 2.0	18a	MOJAVE	0.022$\pm$0.014
3FGL J1224.9+2122	F	0.434	5.32	L18	16.1	0.052	2095	1.97	2.185	2.55E-08	320.4 $\pm$ 9.3	1	MOJAVE	8.41$\pm$0.24
1222+216											581 $\pm$ 17	2a	MOJAVE	15.26$\pm$0.44
											640.6 $\pm$ 8.4	3a	MOJAVE	16.82$\pm$0.22
											638.9 $\pm$ 5.1	4a	MOJAVE	16.77$\pm$0.13
											631.2 $\pm$ 5.8	5a	MOJAVE	16.57$\pm$0.15
											779 $\pm$ 15	6	MOJAVE	20.46$\pm$0.40
											1013 $\pm$ 39	7a	MOJAVE	26.6$\pm$1.0
											632 $\pm$ 45	9	MOJAVE	16.6$\pm$1.2
											444 $\pm$ 35	10	MOJAVE	11.67$\pm$0.92
											615 $\pm$ 23	11	MOJAVE	16.16$\pm$0.60
											96 $\pm$ 19	12	MOJAVE	2.52$\pm$0.49
3FGL J1229.1+0202	F	0.158	3.78	L18	12.9	0.047	54992	63.1	2.516	9.42E-09	829 $\pm$ 45	1	MOJAVE	8.48$\pm$0.46
1226+023											784.1 $\pm$ 5.5	2a	MOJAVE	8.017$\pm$0.056
											1026 $\pm$ 15	3a	MOJAVE	10.49$\pm$0.15
											1255 $\pm$ 54	4	MOJAVE	12.83$\pm$0.56
											1455 $\pm$ 16	5	MOJAVE	14.87$\pm$0.17
											1001 $\pm$ 50	6	MOJAVE	10.23$\pm$0.51
											655 $\pm$ 38	7	MOJAVE	6.70$\pm$0.39
											509 $\pm$ 67	8	MOJAVE	5.20$\pm$0.69
											1013.3 $\pm$ 6.8	9a	MOJAVE	10.360$\pm$0.070
											887.1 $\pm$ 8.1	12a	MOJAVE	9.070$\pm$0.082
											600 $\pm$ 28	13	MOJAVE	6.14$\pm$0.29
											849 $\pm$ 25	15	MOJAVE	8.68$\pm$0.26
											611 $\pm$ 33	16a	MOJAVE	6.24$\pm$0.34
											713 $\pm$ 33	19a	MOJAVE	7.29$\pm$0.34
											538 $\pm$ 15	21	MOJAVE	5.50$\pm$0.15
											664 $\pm$ 47	22	MOJAVE	6.79$\pm$0.48
											716 $\pm$ 24	24	MOJAVE	7.32$\pm$0.25
											513 $\pm$ 26	25a	MOJAVE	5.24$\pm$0.26
											878.3 $\pm$ 5.0	26a	MOJAVE	8.980$\pm$0.051
											1206 $\pm$ 49	27a	MOJAVE	12.33$\pm$0.51
											928 $\pm$ 33	29a	MOJAVE	9.49$\pm$0.33
3FGL J1239.5+0443	F	1.759			20.4	0.051	354	0.28	2.204	5.58E-09	23.1 $\pm$ 10.0	1	MOJAVE	1.78$\pm$0.77
1236+049											32.1 $\pm$ 5.6	2	MOJAVE	2.47$\pm$0.43
3FGL J1246.7-2547	F	0.633			15.9	0.197	1165	1.32	2.14	9.79E-09	115 $\pm$ 56	1a	MOJAVE	4.2$\pm$2.0
1244-255											16 $\pm$ 30	2	MOJAVE	0.6$\pm$1.1
											89 $\pm$ 22	3	MOJAVE	3.23$\pm$0.82
3FGL J1256.1-0547	F	0.536	11.64	L18	15	0.065	9711	20.9	2.233	2.06E-08	348.4 $\pm$ 2.2	1	MOJAVE	11.014$\pm$0.069
1253-055											254 $\pm$ 12	2	MOJAVE	8.05$\pm$0.38
											212 $\pm$ 25	3	MOJAVE	6.70$\pm$0.78
											5.7 $\pm$ 1.5	4a	MOJAVE	0.181$\pm$0.047
											492.6 $\pm$ 9.3	6a	MOJAVE	15.58$\pm$0.30
											651 $\pm$ 25	7	MOJAVE	20.58$\pm$0.79
											304 $\pm$ 17	8a	MOJAVE	9.60$\pm$0.54
											516 $\pm$ 13	10	MOJAVE	16.30$\pm$0.40
											468 $\pm$ 61	11	MOJAVE	14.8$\pm$1.9
3FGL J1308.7+3545	F	1.055	24.99	L18	20	0.021	239	0.23	2.357	5.53E-10	84	C1	CJF	4.26$\pm$0
1306+360
3FGL J1310.6+3222	F	0.998	26.35	L18	17.6	0.033	1687	0.53	2.153	3.65E-09	444 $\pm$ 18	1	MOJAVE	23.21$\pm$0.93
1308+326											407.1 $\pm$ 8.3	2	MOJAVE	21.31$\pm$0.43
											442 $\pm$ 46	3	MOJAVE	23.2$\pm$2.4
											525 $\pm$ 22	4	MOJAVE	27.5$\pm$1.2
											401.8 $\pm$ 5.6	5	MOJAVE	21.03$\pm$0.29
											340 $\pm$ 30	7	MOJAVE	17.8$\pm$1.6
											202 $\pm$ 20	8a	MOJAVE	10.6$\pm$1.0
											159.6 $\pm$ 4.9	9a	MOJAVE	8.35$\pm$0.26
											350.4 $\pm$ 9.2	11a	MOJAVE	18.34$\pm$0.48
											58 $\pm$ 23	12	MOJAVE	3.1$\pm$1.2
											237 $\pm$ 59	13	MOJAVE	12.4$\pm$3.1
3FGL J1332.0-0508	F	2.15	26.11	L18	18.4	0.066	527	0.29	2.454	4.68E-09	23 $\pm$ 114	1	MOJAVE	1.9$\pm$9.9
1329-049											76 $\pm$ 16	2	MOJAVE	6.5$\pm$1.4
3FGL J1337.6-1257	F	0.539	5.3	L18	17.8	0.174	2676	1.77	2.366	1.56E-09	466 $\pm$ 21	5	MOJAVE	14.80$\pm$0.68
1334-0127											343 $\pm$ 14	9	MOJAVE	10.91$\pm$0.43
											483 $\pm$ 37	10	MOJAVE	15.4$\pm$1.2
											503 $\pm$ 31	11a	MOJAVE	15.98$\pm$0.98
											308 $\pm$ 29	12	MOJAVE	9.80$\pm$0.92
											690 $\pm$ 35	13	MOJAVE	21.9$\pm$1.1
3FGL J1345.6+4453	F	2.534			20.3	0.053	294	0.2	2.195	6.52E-09	118 $\pm$ 25	2	MOJAVE	11.1$\pm$2.4
1343+451
3FGL J1350.8+3035	F	0.712	16.8	L18	17.9	0.035	322	0.91	2.371	1.04E-09	367 $\pm$ 19	1	MOJAVE	14.74$\pm$0.76
1348+308											373 $\pm$ 40	2	MOJAVE	15.0$\pm$1.6
3FGL J1408.8-0751	F	1.49			18.6	0.079	689	0.53	2.3798	1.79E-09	247.9 $\pm$ 8.9	2	MOJAVE	17.22$\pm$0.62
1406?076											171 $\pm$ 17	3	MOJAVE	11.9$\pm$1.2
											292 $\pm$ 19	8	MOJAVE	20.3$\pm$1.3
											70.7 $\pm$ 4.0	9	MOJAVE	4.91$\pm$0.28
											326 $\pm$ 11	11a	MOJAVE	22.64$\pm$0.77
3FGL J1416.0+1325	F	0.247	8.59	L18	19.1	0.056	1092	0.04	2.363	5.30E-10	30 $\pm$ 23	1	MOJAVE	0.47$\pm$0.37
PKS B1413+135											18 $\pm$ 13	2	MOJAVE	0.29$\pm$0.21
											94.7 $\pm$ 5.8	3a	MOJAVE	1.481$\pm$0.090
											77.0 $\pm$ 9.4	4	MOJAVE	1.20$\pm$0.15
											7.2 $\pm$ 4.8e	6	MOJAVE	0.112$\pm$0.074
											0.0 $\pm$ 4.3	7a	MOJAVE	0.000$\pm$0.067
											9.4 $\pm$ 2.3e	8	MOJAVE	0.147$\pm$0.035
3FGL J1419.8+3819	F	1.831	32.39	L18	19.3	0.018	612	0.2	2.365	5.99E-10	196 $\pm$ 38	1	MOJAVE	15.4$\pm$3.0
B3 1417+385											89 $\pm$ 14	3	MOJAVE	7.0$\pm$1.1
3FGL J1419.9+5425	B	0.153	9.89	L18	15.4	0.031	789	0.81	2.307	9.65E-10	390	K2	X95	3.63
1418+546
3FGL J1427.0+2347	B	0.16			14.6	0.13	430	3.57	1.76	1.36E-08	18 $\pm$ 75	1	MOJAVE	0.6$\pm$2.6
1424+240											74 $\pm$ 30	2	MOJAVE	2.6$\pm$1.1
3FGL J1434.1+4203	F	1.24	28.41	L18	19.5	0.038	309	0	2.392	3.64E-10	287$\pm$11	C1	CJF	16.31$\pm$0.63
B3 1432+422
3FGL J1504.4+1029	F	1.84	17.65	L18	18.2	0.074	1774	0.16	2.075	2.40E-08	132.6 $\pm$ 6.6	2	MOJAVE	10.48$\pm$0.52
PKS 1502+106											78 $\pm$ 13	3	MOJAVE	6.2$\pm$1.0
											231 $\pm$ 14	4	MOJAVE	18.3$\pm$1.1
											61.2 $\pm$ 2.8	5a	MOJAVE	4.84$\pm$0.22
3FGL J1505.1+0326	F	0.408	18.23	L18	18.2	0.105	395	0.1	2.609	1.27E-09	46 $\pm$ 15	4	MOJAVE	1.14$\pm$0.38
1502+036
3FGL J1506.1+3728	F	0.672	14.49	L18	21.2	0.031	938	0.37	2.453	7.64E-10	274$\pm$43	C1	CJF	9.8$\pm$1.54
B2 1504+37											171$\pm$42	C2	CJF	6.12$\pm$1.5
											250	C3	CJF	8.94$\pm$0
											95$\pm$86	C4	CJF	3.4$\pm$3.08
3FGL J1510.9-0542	F	1.185	1.7	L18	16.9	0.192	3570	0.42	2.426	1.99E-09	4 $\pm$ 16	2	MOJAVE	0.23$\pm$0.95
1508-055											18.2 $\pm$ 7.3	4	MOJAVE	1.09$\pm$0.43
3FGL J1512.8-0906	F	0.36	32.14	L18	15.7	0.229	2701	1.15	2.305	4.11E-08	722 $\pm$ 18	1a	MOJAVE	16.01$\pm$0.39
1510-089											831 $\pm$ 108	2	MOJAVE	18.4$\pm$2.4
											211 $\pm$ 50	3	MOJAVE	4.7$\pm$1.1
											908 $\pm$ 48	4	MOJAVE	20.1$\pm$1.1
											824 $\pm$ 82	5	MOJAVE	18.3$\pm$1.8
											666 $\pm$ 41	6	MOJAVE	14.77$\pm$0.92
											1042 $\pm$ 22	8a	MOJAVE	23.12$\pm$0.49
											765 $\pm$ 117	9	MOJAVE	17.0$\pm$2.6
											972 $\pm$ 22	15	MOJAVE	21.55$\pm$0.49
											1263 $\pm$ 27	16a	MOJAVE	28.00$\pm$0.60
											1038 $\pm$ 39	17a	MOJAVE	23.03$\pm$0.85
											952 $\pm$ 18	19a	MOJAVE	21.11$\pm$0.40
											161 $\pm$ 50	20	MOJAVE	3.6$\pm$1.1
											1126 $\pm$ 104	22	MOJAVE	25.0$\pm$2.3
3FGL J1516.9+1926	B	1.07	9.71	L18	18.4	0.091	465	0.27	2.768	2.80E-10	54 $\pm$ 33	1	MOJAVE	3.0$\pm$1.8
1514+197											178 $\pm$ 24	2	MOJAVE	9.8$\pm$1.3
											375 $\pm$ 37	3	MOJAVE	20.7$\pm$2.0
3FGL J1517.6-2422	B	0.049			12.6	0.315	2042	1.05	2.112	5.23E-09	1711 $\pm$ 111	8	MOJAVE	5.54$\pm$0.36
1514-241											1930 $\pm$ 56	9a	MOJAVE	6.25$\pm$0.18
											1919 $\pm$ 81	10	MOJAVE	6.21$\pm$0.26
3FGL J1522.1+3144	F	1.487	35.22	L18	19.8	0.053	348	0.23	2.247	1.79E-08	18.1 $\pm$ 5.9	2	MOJAVE	1.26$\pm$0.41
1520+319											23 $\pm$ 17	3	MOJAVE	1.6$\pm$1.2
3FGL J1540.8+1449	B	0.605	8.64	L18	18.1	0.124	1387	0.84	2.345	3.70E-10	23 $\pm$ 16	1	MOJAVE	0.82$\pm$0.55
1538+149											249 $\pm$ 27	2	MOJAVE	8.73$\pm$0.97
											150 $\pm$ 17	3	MOJAVE	5.28$\pm$0.61
											13.7 $\pm$ 1.6e	4	MOJAVE	0.483$\pm$0.057
											154 $\pm$ 51	6	MOJAVE	5.4$\pm$1.8
3FGL J1549.4+0237	F	0.414	10.75	L18	17.3	0.259	836	1.2	2.463	1.76E-09	480 $\pm$ 50	2	MOJAVE	12.1$\pm$1.2
PKS 1546+027											438 $\pm$ 25	3	MOJAVE	11.03$\pm$0.63
											166 $\pm$ 22	4	MOJAVE	4.19$\pm$0.55
											364 $\pm$ 11	6a	MOJAVE	9.16$\pm$0.27
											382 $\pm$ 11	7a	MOJAVE	9.60$\pm$0.28
											235 $\pm$ 16	8	MOJAVE	5.93$\pm$0.41
3FGL J1550.5+0526	F	1.442	4.16	L18	18.3	0.157	2304	0.94	2.336	1.26E-09	172 $\pm$ 25	1	MOJAVE	11.6$\pm$1.7
1548+056											159 $\pm$ 18	3	MOJAVE	10.7$\pm$1.2
											77 $\pm$ 16	7	MOJAVE	5.2$\pm$1.1
											112.4 $\pm$ 4.1	8	MOJAVE	7.54$\pm$0.28
3FGL J1553.5+1256	F	1.29			17.3	0.096	948	0.29	2.223	2.76E-09	26 $\pm$ 25	1	MOJAVE	1.6$\pm$1.6
1551+130											137 $\pm$ 85	2	MOJAVE	8.7$\pm$5.4
											17 $\pm$ 39	3	MOJAVE	1.1$\pm$2.5
											43.7 $\pm$ 7.9	4	MOJAVE	2.78$\pm$0.50
											42 $\pm$ 16	5	MOJAVE	2.7$\pm$1.0
											129 $\pm$ 80	6	MOJAVE	8.2$\pm$5.1
3FGL J1608.6+1029	F	1.232	8.38	L18	18.1	0.136	1392	0.53	2.619	1.29E-09	296 $\pm$ 14	5	MOJAVE	18.05$\pm$0.83
1606+106											259 $\pm$ 32	6	MOJAVE	15.8$\pm$1.9
											294 $\pm$ 15	7	MOJAVE	17.97$\pm$0.92
											106 $\pm$ 12	8	MOJAVE	6.47$\pm$0.72
3FGL J1613.8+3410	F	1.4	4.63	L18	17.3	0.041	4024	0.4	2.352	6.52E-10	74.9 $\pm$ 2.2	4a	MOJAVE	4.99$\pm$0.14
1611+343											467 $\pm$ 29	5	MOJAVE	31.1$\pm$1.9
											207 $\pm$ 12	9	MOJAVE	13.76$\pm$0.80
											230 $\pm$ 12	10	MOJAVE	15.28$\pm$0.83
											48.9 $\pm$ 5.6	13	MOJAVE	3.26$\pm$0.37
											81.8 $\pm$ 9.2	15	MOJAVE	5.44$\pm$0.61
											48 $\pm$ 41	19	MOJAVE	3.2$\pm$2.7
3FGL J1625.7-2527	F	0.786			20.6	2.816	2521	0.36	2.2318	1.12E-08	510$\pm$130		JM01	20.71$\pm$5.28
1622?253
3FGL J1626.0-2951	F	0.815			17.6	1.5	2286	0.59	2.507	2.50E-09	108 $\pm$ 29	1	MOJAVE	4.8$\pm$1.3
1622?297											268 $\pm$ 30	2	MOJAVE	12.0$\pm$1.4
											94 $\pm$ 41	3	MOJAVE	4.2$\pm$1.8
											62 $\pm$ 30	4	MOJAVE	2.8$\pm$1.4
3FGL J1635.2+3809	F	1.813	26.96	L18	17.6	0.027	2726	0.17	2.414	1.14E-08	256 $\pm$ 13	2a	MOJAVE	20.0$\pm$1.0
1633+382											286 $\pm$ 15	3a	MOJAVE	22.4$\pm$1.1
											373 $\pm$ 16	4	MOJAVE	29.3$\pm$1.3
											292 $\pm$ 13	5a	MOJAVE	22.9$\pm$1.0
											104 $\pm$ 13	8a	MOJAVE	8.1$\pm$1.0
											28.5 $\pm$ 5.7	10	MOJAVE	2.23$\pm$0.44
											172 $\pm$ 15	16a	MOJAVE	13.5$\pm$1.2
											82 $\pm$ 14	17	MOJAVE	6.4$\pm$1.1
											125.3 $\pm$ 7.2	18	MOJAVE	9.82$\pm$0.56
											39.6 $\pm$ 4.6	19a	MOJAVE	3.10$\pm$0.36
3FGL J1637.7+4715	F	0.74	20.85	L18	18.8	0.051	19	0.1	2.368	1.77E-09	15 $\pm$ 24e	1	MOJAVE	0.6$\pm$1.0
1636+473											229.0 $\pm$ 7.4	2	MOJAVE	9.44$\pm$0.30
											235.2 $\pm$ 8.7	3	MOJAVE	9.70$\pm$0.36
											113.1 $\pm$ 7.1	4	MOJAVE	4.66$\pm$0.29
3FGL J1640.6+3945	F	1.66	31.29	L18	19.5	0.024	976	0.15	2.285	3.91E-09	222 $\pm$ 22	1	MOJAVE	16.5$\pm$1.6
1638+398
3FGL J1642.9+3950	F	0.593	4.63	L18	15.4	0.03	7099	2.52	2.447	2.51E-09	261 $\pm$ 24	1	MOJAVE	9.00$\pm$0.84
1641+399											253 $\pm$ 11	2a	MOJAVE	8.72$\pm$0.39
											320.3 $\pm$ 8.0	3a	MOJAVE	11.05$\pm$0.28
											332 $\pm$ 13	4	MOJAVE	11.46$\pm$0.44
											408 $\pm$ 23	5a	MOJAVE	14.06$\pm$0.78
											338.9 $\pm$ 4.4	6a	MOJAVE	11.69$\pm$0.15
											368.3 $\pm$ 2.4	7a	MOJAVE	12.699$\pm$0.081
											337.4 $\pm$ 2.8	8a	MOJAVE	11.636$\pm$0.095
											348.6 $\pm$ 4.2	9	MOJAVE	12.02$\pm$0.14
											559 $\pm$ 15	11	MOJAVE	19.29$\pm$0.51
											382 $\pm$ 11	12a	MOJAVE	13.16$\pm$0.37
											263 $\pm$ 10	13	MOJAVE	9.06$\pm$0.36
											321 $\pm$ 19	15	MOJAVE	11.06$\pm$0.64
											231 $\pm$ 53	18	MOJAVE	8.0$\pm$1.8
											101 $\pm$ 26	19a	MOJAVE	3.47$\pm$0.91
											383 $\pm$ 32	21	MOJAVE	13.2$\pm$1.1
3FGL J1653.9+3945	B	0.034	0.23	L18	13.3	0.044	1558	36.9	1.716	9.74E-09	960 $\pm$ 100		JM01	2.05$\pm$0.21
1652+398
3FGL J1657.7+4807	F	1.669	26.23	L18	21.7	0.046	1036	0.12	2.476	1.38E-09	144 $\pm$ 50	1	MOJAVE	10.8$\pm$3.7
1656+482											257 $\pm$ 29	2	MOJAVE	19.1$\pm$2.1
											23 $\pm$ 21	3	MOJAVE	1.7$\pm$1.6
3FGL J1700.1+6829	F	0.301	15.11	L18	18.4	0.105	338	0.15	2.398	2.98E-09	445 $\pm$ 23	3	MOJAVE	8.38$\pm$0.42
1700+685											398 $\pm$ 27	4	MOJAVE	7.49$\pm$0.50
											591 $\pm$ 39	6	MOJAVE	11.11$\pm$0.72
											148 $\pm$ 22	8	MOJAVE	2.79$\pm$0.41
3FGL J1710.6+4317	F	1.027	32.46	L18	19	0.039	143	0.1	2.527	1.31E-09	35 $\pm$ 53	2	MOJAVE	1.9$\pm$2.9
1708+433											100 $\pm$ 33	3	MOJAVE	5.4$\pm$1.8
											96 $\pm$ 13	4	MOJAVE	5.13$\pm$0.69
3FGL J1723.9+4004	F	1.049	3.94	L18	21	0.08	568	0	2.452	1.18E-09	322 $\pm$ 86	1	MOJAVE	17.5$\pm$4.7
1722+401											609 $\pm$ 59	2	MOJAVE	33.1$\pm$3.2
											220 $\pm$ 17	3	MOJAVE	11.96$\pm$0.94
3FGL J1727.1+4531	F	0.717	24	L18	18.5	0.057	914	0.27	2.347	1.40E-09	52 $\pm$ 17	2	MOJAVE	2.11$\pm$0.68
S4 1726+45											57.3 $\pm$ 5.1	3	MOJAVE	2.32$\pm$0.20
											49.9 $\pm$ 8.2	4	MOJAVE	2.02$\pm$0.33
3FGL J1728.5+0428	F	0.296	11.5	L18	17.7	0.341	682	0.44	2.954	8.96E-10	506 $\pm$ 45	1	MOJAVE	9.28$\pm$0.83
1725+044											510 $\pm$ 43	2a	MOJAVE	9.35$\pm$0.79
											378 $\pm$ 21	3	MOJAVE	6.94$\pm$0.39
											589 $\pm$ 10	4a	MOJAVE	10.80$\pm$0.19
											236 $\pm$ 11	8	MOJAVE	4.32$\pm$0.20
3FGL J1733.0-1305	F	0.902	21.48	L18	17.8	1.187	5990	1.64	2.245	5.59E-09	128 $\pm$ 15	1	MOJAVE	6.19$\pm$0.72
1730-130											360 $\pm$ 14	2a	MOJAVE	17.46$\pm$0.67
											564 $\pm$ 20	4a	MOJAVE	27.35$\pm$0.97
											283.2 $\pm$ 8.2	6	MOJAVE	13.74$\pm$0.40
											184 $\pm$ 21	7	MOJAVE	8.90$\pm$1.00
											348 $\pm$ 13	8a	MOJAVE	16.89$\pm$0.62
3FGL J1734.3+3858	F	0.975	34.26	L18	19.5	0.108	796	0.13	2.313	2.33E-09	245 $\pm$ 36	4	MOJAVE	12.6$\pm$1.8
1732+389											197 $\pm$ 30	6	MOJAVE	10.1$\pm$1.5
											166 $\pm$ 27	7	MOJAVE	8.5$\pm$1.4
3FGL J1739.4+4955	F	1.545	15.03	L18	18.2	0.056	531	0.26	2.307	1.29E-09	166 $\pm$ 56	1	MOJAVE	11.8$\pm$4.0
1738+499											42 $\pm$ 14	2	MOJAVE	3.0$\pm$1.0
3FGL J1740.3+5211	F	1.379	20.43	L18	17.2	0.081	807	0.58	2.453	1.67E-09	173$\pm$136	C1	CJF	10.56$\pm$8.3
1739+522
3FGL J1748.6+7005	B	0.77	12.04	L18	15.6	0.068	735	0.72	2.064	4.14E-09	23.8 $\pm$ 3.5	2a	MOJAVE	1.02$\pm$0.15
1749+701											24.8 $\pm$ 3.1	3a	MOJAVE	1.06$\pm$0.13
											7.2 $\pm$ 1.5	5	MOJAVE	0.308$\pm$0.063
3FGL J1751.5+0939	B	0.322	17.62	L18	17	0.406	623	1.18	2.118	4.25E-09	139 $\pm$ 23	4	MOJAVE	2.77$\pm$0.47
1749+096											121 $\pm$ 18	5a	MOJAVE	2.42$\pm$0.36
											395 $\pm$ 38	8	MOJAVE	7.90$\pm$0.75
3FGL J1800.5+7827	B	0.68	36.56	L18	17.1	0.119	2223	0.79	2.223	5.07E-09	242 $\pm$ 23	1a	MOJAVE	9.36$\pm$0.87
1803+784											29.8 $\pm$ 7.8	2	MOJAVE	1.15$\pm$0.30
											15.3 $\pm$ 2.4	3a	MOJAVE	0.591$\pm$0.092
											9.9 $\pm$ 1.5	4a	MOJAVE	0.383$\pm$0.057
											4.8 $\pm$ 3.1	5a	MOJAVE	0.18$\pm$0.12
											1.22 $\pm$ 0.86	6a	MOJAVE	0.047$\pm$0.033
3FGL J1801.5+4403	F	0.663	21.56	L18	15.7	0.137	727	0.68	2.695	4.82E-10	396 $\pm$ 13	3	MOJAVE	15.01$\pm$0.48
1800+440											395 $\pm$ 28	4	MOJAVE	14.9$\pm$1.0
											385 $\pm$ 16	10	MOJAVE	14.57$\pm$0.61
											335 $\pm$ 24	11	MOJAVE	12.70$\pm$0.90
											447 $\pm$ 37	12	MOJAVE	16.9$\pm$1.4
3FGL J1824.2+5649	B	0.664	17.35	L18	17.5	0.144	1412	1.17	2.46	2.01E-09	234 $\pm$ 36	1	MOJAVE	8.9$\pm$1.4
1823+568											138 $\pm$ 15	2	MOJAVE	5.25$\pm$0.57
											483.9 $\pm$ 8.1	4a	MOJAVE	18.35$\pm$0.31
											207.0 $\pm$ 7.6	6a	MOJAVE	7.85$\pm$0.29
											132 $\pm$ 11	8	MOJAVE	5.02$\pm$0.43
											2.9 $\pm$ 1.1e	9	MOJAVE	0.108$\pm$0.041
											142 $\pm$ 26	10	MOJAVE	5.40$\pm$0.99
											87.9 $\pm$ 7.0	12	MOJAVE	3.33$\pm$0.27
											576 $\pm$ 48	14	MOJAVE	21.9$\pm$1.8
											81 $\pm$ 34	15	MOJAVE	3.1$\pm$1.3
											0.5 $\pm$ 3.6e	16	MOJAVE	0.02$\pm$0.13
3FGL J1829.6+4844	SY1.5	0.692	20.9	L18	16.7	0.178	13753	2.2	2.365	1.49E-09	120 $\pm$ 15	1	MOJAVE	4.72$\pm$0.60
1828+487											280.6 $\pm$ 8.2	2a	MOJAVE	11.01$\pm$0.32
											252.2 $\pm$ 4.2	3a	MOJAVE	9.90$\pm$0.17
											331.8 $\pm$ 8.7	5	MOJAVE	13.02$\pm$0.34
											322 $\pm$ 11	6	MOJAVE	12.65$\pm$0.45
											332.9 $\pm$ 3.7	8a	MOJAVE	13.07$\pm$0.14
											9.0 $\pm$ 4.2e	9	MOJAVE	0.35$\pm$0.17
											125 $\pm$ 10	10a	MOJAVE	4.90$\pm$0.41
3FGL J1830.1+0617	F	0.75	22.64	L18	19.5	1.068	397	0.32	2.11	1.68E-09	317 $\pm$ 35	2	MOJAVE	13.2$\pm$1.4
1827+062											97 $\pm$ 13	3	MOJAVE	4.03$\pm$0.54
											89.4 $\pm$ 8.7	4	MOJAVE	3.73$\pm$0.36
											8.9 $\pm$ 8.7e	5	MOJAVE	0.37$\pm$0.36
3FGL J1848.4+3216	F	0.798	23.02	L18	18.9	0.227	516	1	2.412	2.43E-09	96 $\pm$ 26	1	MOJAVE	4.3$\pm$1.2
1846+322											27.0 $\pm$ 6.0	2	MOJAVE	1.19$\pm$0.26
3FGL J1849.2+6705	F	0.657	28.89	L18	17.5	0.129	517	0.41	2.143	4.97E-09	316 $\pm$ 23	1	MOJAVE	11.90$\pm$0.85
1849+670											570 $\pm$ 37	3	MOJAVE	21.4$\pm$1.4
											556 $\pm$ 20	4a	MOJAVE	20.91$\pm$0.77
											331 $\pm$ 33	6	MOJAVE	12.4$\pm$1.3
											53 $\pm$ 10	7	MOJAVE	1.99$\pm$0.39
3FGL J1911.2-2006	F	0.2			18.9	0.371	2714	1.77	2.409	3.72E-09	77 $\pm$ 21	1	MOJAVE	4.4$\pm$1.2
1908?201											45.8 $\pm$ 7.4	2	MOJAVE	2.61$\pm$0.42
3FGL J1923.5-2104	F	0.874			16.6	0.234	3167	0.77	1.998	4.67E-09	38 $\pm$ 14	2	MOJAVE	1.81$\pm$0.68
1920-211											186 $\pm$ 15	3	MOJAVE	8.78$\pm$0.71
3FGL J1924.8-2914	F	0.363			17.3	0.29	13387	2.42	2.503	2.16E-09	275 $\pm$ 33	1	MOJAVE	5.99$\pm$0.72
1921-293
3FGL J1954.8-1122	F	0.683	29.56	L18	18.9	0.358	367	0.34	2.271	2.14E-09	186 $\pm$ 17	2	MOJAVE	7.22$\pm$0.68
1951-115
3FGL J2005.2+7752	B	0.342	1.27	L18	16.1	0.362	1061	0.43	2.219	F	180 $\pm$ 40	C2	VC94	3.58$\pm$0.8
2007+777
3FGL J2015.6+3709	F		20.3	O16	21.4	4.154	2167	0.66	2.535	9.32E-09	146 $\pm$ 11	1a	MOJAVE	6.83$\pm$0.50
2013+370											306.0 $\pm$ 6.0	2a	MOJAVE	14.29$\pm$0.28
											18.1 $\pm$ 6.2e	4	MOJAVE	0.84$\pm$0.29
3FGL J2023.2+3154	Un		6	O16					2.072	8.12E-10	117 $\pm$ 18	2	MOJAVE	2.56$\pm$0.38
2021+317											45.5 $\pm$ 8.4	4	MOJAVE	1.00$\pm$0.18
											18.0 $\pm$ 7.6e	8	MOJAVE	0.39$\pm$0.17
											208 $\pm$ 11	9a	MOJAVE	4.56$\pm$0.24
											174 $\pm$ 15	10	MOJAVE	3.83$\pm$0.33
											94.9 $\pm$ 7.3	11	MOJAVE	2.08$\pm$0.16
3FGL J2025.6-0736	F	1.388	21.74	L18	18.7	0.087	1347	0.65	2.182	6.97E-09	291 $\pm$ 15	5	MOJAVE	19.26$\pm$0.98
2022-077
3FGL J2031.8+1223	B	1.215	11.86	L18	17.4	0.183	999	0.19	2.445	7.47E-10	190 $\pm$ 35	8	MOJAVE	11.4$\pm$2.1
2029+121
3FGL J2115.4+2933	F	1.514	11.25	L18	18.9	0.296	756	0.15	2.373	1.24E-09	88 $\pm$ 10	6	MOJAVE	6.19$\pm$0.73
B2 2113+29
3FGL J2134.1-0152	B	1.284	9.31	L18	17.6	0.124	1691	0.32	2.207	1.12E-09	195 $\pm$ 11	1a	MOJAVE	12.22$\pm$0.69
PKS 2131-021											318 $\pm$ 22	2	MOJAVE	19.9$\pm$1.4
											169.3 $\pm$ 4.9	3a	MOJAVE	10.63$\pm$0.31
											40.8 $\pm$ 2.8	4a	MOJAVE	2.56$\pm$0.18
											3.0 $\pm$ 1.7e	5	MOJAVE	0.19$\pm$0.11
3FGL J2143.5+1744	F	0.21	15.46	L18	16	0.261	652	0.67	2.404	4.42E-09	108 $\pm$ 22	2	MOJAVE	1.45$\pm$0.30
2141+175											157 $\pm$ 22	5	MOJAVE	2.11$\pm$0.30
3FGL J2158.0-1501	F	0.672	29.14	L18	17.3	0.113	3021	0.81	2.269	1.06E-09	52.0 $\pm$ 9.0	1	MOJAVE	1.99$\pm$0.35
PKS 2155-152											473 $\pm$ 46	2	MOJAVE	18.1$\pm$1.8
											241 $\pm$ 11	3	MOJAVE	9.25$\pm$0.41
											28.5 $\pm$ 9.5	4a	MOJAVE	1.09$\pm$0.36
3FGL J2202.7+4217	B	0.069	7.2	S10	12.5	0.751	6051	10.4	2.161	1.65E-08	2205 $\pm$ 159	1	MOJAVE	9.96$\pm$0.72
2200+420											1760 $\pm$ 158	2	MOJAVE	7.94$\pm$0.71
											930 $\pm$ 57	3a	MOJAVE	4.20$\pm$0.26
											1332 $\pm$ 47	4a	MOJAVE	6.01$\pm$0.21
											778 $\pm$ 29	5a	MOJAVE	3.51$\pm$0.13
											684 $\pm$ 27	6a	MOJAVE	3.09$\pm$0.12
											3.76 $\pm$ 0.64	7a	MOJAVE	0.017$\pm$0.0029
											1577 $\pm$ 121	8	MOJAVE	7.12$\pm$0.55
											1002 $\pm$ 61	10	MOJAVE	4.52$\pm$0.28
											2042 $\pm$ 50	11a	MOJAVE	9.22$\pm$0.23
											1234 $\pm$ 57	12	MOJAVE	5.57$\pm$0.26
											1082 $\pm$ 38	13	MOJAVE	4.89$\pm$0.17
											1001 $\pm$ 119	14	MOJAVE	4.52$\pm$0.54
											823 $\pm$ 51	15	MOJAVE	3.71$\pm$0.23
											904 $\pm$ 28	16a	MOJAVE	4.08$\pm$0.13
											1557 $\pm$ 94	19	MOJAVE	7.03$\pm$0.42
											458 $\pm$ 36	24	MOJAVE	2.07$\pm$0.16
											1598 $\pm$ 159	28	MOJAVE	7.22$\pm$0.72
											2114 $\pm$ 93	34	MOJAVE	9.55$\pm$0.42
3FGL J2203.4+1725	F	1.076	34.58	L18	17	0.128	593	0.46	2.152	4.75E-09	17.9 $\pm$ 4.0e	1	MOJAVE	0.99$\pm$0.22
PKS 2201+171											285 $\pm$ 30	5	MOJAVE	15.8$\pm$1.7
											317 $\pm$ 20	7	MOJAVE	17.6$\pm$1.1
3FGL J2212.0+2355	F	1.125	12.33	L18	19.6	0.166	557	0.33	2.212	1.10E-09	23.7 $\pm$ 5.0	4a	MOJAVE	1.35$\pm$0.28
PKS 2209+236											6.1 $\pm$ 1.6	5	MOJAVE	0.351$\pm$0.094
3FGL J2225.8-0454	F	1.404	4.38	L18	17.6	0.173	7412	0.89	2.359	1.94E-09	224 $\pm$ 19	1	MOJAVE	15.0$\pm$1.3
2223-052											130.7 $\pm$ 7.0	2a	MOJAVE	8.72$\pm$0.46
											260.7 $\pm$ 7.2	4a	MOJAVE	17.39$\pm$0.48
											217.9 $\pm$ 6.8	5	MOJAVE	14.53$\pm$0.45
											202 $\pm$ 11	8	MOJAVE	13.49$\pm$0.75
											196 $\pm$ 17	9a	MOJAVE	13.1$\pm$1.1
											266 $\pm$ 46	10	MOJAVE	17.7$\pm$3.1
											11 $\pm$ 13e	12	MOJAVE	0.72$\pm$0.87
3FGL J2229.7-0833	F	1.56	20.88	L18	17.1	0.116	969	1.43	2.389	3.53E-09	3 $\pm$ 12e	3	MOJAVE	0.24$\pm$0.86
PKS 2227-08											42.6 $\pm$ 6.9	4	MOJAVE	3.04$\pm$0.50
3FGL J2232.5+1143	F	1.037	13.39	L18	16.7	0.165	7202	1.26	2.339	5.02E-09	79 $\pm$ 21	1	MOJAVE	4.3$\pm$1.1
2230+114											160.3 $\pm$ 8.0	2	MOJAVE	8.64$\pm$0.43
											14.2 $\pm$ 6.5e	3	MOJAVE	0.77$\pm$0.35
											21.6 $\pm$ 2.3	4	MOJAVE	1.16$\pm$0.12
											329 $\pm$ 16	16	MOJAVE	17.73$\pm$0.87
											86 $\pm$ 10	19a	MOJAVE	4.66$\pm$0.55
3FGL J2236.3+2829	B	0.795	20.19	L18	17.2	0.147	1103	0.61	2.115	4.30E-09	74.6 $\pm$ 6.8	5	MOJAVE	3.26$\pm$0.30
2234+282
3FGL J2236.5-1432	B	0.325			19.2	0.101	542	0.42	2.043	6.86E-09	45 $\pm$ 41	2	MOJAVE	0.91$\pm$0.84
2233-148											71 $\pm$ 35	3	MOJAVE	1.43$\pm$0.70
3FGL J2244.1+4057	B	1.171	51.71	L18	19.7	0.383	227	0	2.289	1.65E-09	240 $\pm$ 50	2	MOJAVE	14.1$\pm$3.0
2241+406
3FGL J2250.7-2806	F	0.525			19.3	0.05	306	0.34	2.177	4.15E-09	583 $\pm$ 58	6	MOJAVE	18.1$\pm$1.8
2247-283
3FGL J2254.0+1608	F	0.859	26.61	L18	13.2	0.241	12657	7.8	1.635	1.06E-07	41.9 $\pm$ 8.0	1a	MOJAVE	1.95$\pm$0.37
2251+158											85.3 $\pm$ 3.1	2	MOJAVE	3.98$\pm$0.14
											203.7 $\pm$ 8.7	3	MOJAVE	9.51$\pm$0.41
											286.0 $\pm$ 5.7	4a	MOJAVE	13.35$\pm$0.27
											198.2 $\pm$ 9.3	5a	MOJAVE	9.26$\pm$0.43
											295 $\pm$ 10	8a	MOJAVE	13.80$\pm$0.49
											74 $\pm$ 18	13	MOJAVE	3.46$\pm$0.86
3FGL J2258.0-2759	F	0.926			17.2	0.077	1249	1	2.173	4.33E-09	82.8 $\pm$ 7.4	1	MOJAVE	4.10$\pm$0.37
2255-282
3FGL J2311.0+3425	F	1.817			18.3	0.185	980	0.3	2.192	5.34E-09	22 $\pm$ 20	2	MOJAVE	1.8$\pm$1.6
2308+341											46 $\pm$ 37	3	MOJAVE	3.6$\pm$2.9
3FGL J2321.9+3204	F	1.489	32.92	L18	20	0.31	253	0.16	2.07	2.13E-09	171 $\pm$ 16	1	MOJAVE	11.9$\pm$1.1
2319+317											53 $\pm$ 17	2	MOJAVE	3.7$\pm$1.2
3FGL J2323.5-0315	F	1.41	51.71	L18	18.3	0.096	928	0.51	2.157	3.03E-09	82 $\pm$ 84	1	MOJAVE	5.5$\pm$5.6
2320-035											456 $\pm$ 22	2	MOJAVE	30.5$\pm$1.5
											129 $\pm$ 32	5	MOJAVE	8.6$\pm$2.1
3FGL J2327.7+0941	F	1.843	30.83	L18	17.9	0.086	741	0.73	2.678	1.28E-09	38 $\pm$ 21	1	MOJAVE	3.0$\pm$1.6
2325+093											65.9 $\pm$ 6.8	3	MOJAVE	5.21$\pm$0.54
3FGL J2334.1+0732	F	0.401	8.79	L18	17.2	0.191	631	1.06	2.505	6.85E-10	183 $\pm$ 19	1	MOJAVE	4.48$\pm$0.47
TXS 2331+073											176 $\pm$ 11	2	MOJAVE	4.31$\pm$0.27
											219 $\pm$ 30	3	MOJAVE	5.35$\pm$0.74
											323 $\pm$ 22	4	MOJAVE	7.90$\pm$0.53
3FGL J2345.2-1554	F	0.621	30.23	L18	18.5	0.055	226	0.72	2.018	1.14E-08	266 $\pm$ 44	1	MOJAVE	9.5$\pm$1.6
2342-161											120 $\pm$ 21	2	MOJAVE	4.30$\pm$0.76
											69 $\pm$ 17	3a	MOJAVE	2.46$\pm$0.61
3FGL J2348.0-1630	F	0.576	16.58	L18	18.1	0.059	2642	1.29	2.203	2.56E-09	185 $\pm$ 26	1	MOJAVE	6.24$\pm$0.87
PKS 2345-16											341 $\pm$ 23	3	MOJAVE	11.46$\pm$0.76
											246.1 $\pm$ 7.7	4a	MOJAVE	8.28$\pm$0.26
											310 $\pm$ 18	5	MOJAVE	10.44$\pm$0.60
											199 $\pm$ 37	7	MOJAVE	6.7$\pm$1.3
											302 $\pm$ 25	11	MOJAVE	10.17$\pm$0.84
											159 $\pm$ 11	12a	MOJAVE	5.36$\pm$0.38
											262 $\pm$ 21	14	MOJAVE	8.82$\pm$0.71

Table 5. Table 5: Full table of Table 2

FGL name	Class	redshift	${\delta }_R$	Ref	$m_o$	Ext	SR	SX	$\mu$	comp	Ref	$\beta$
Other name					$magnitude$		$mJy$	$1\times {10}^{-12}cgs$	$\mu as/yr$
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)	(10)	(11)	(12)	(13)
0003-066	B	0.347	6.96	L18	17.9	0.087	2051	0.82	191 $\pm$ 15	2	MOJAVE	4.09$\pm$0.33
									250 $\pm$ 39	3	MOJAVE	5.36$\pm$0.83
									50.4 $\pm$ 5.3	4a	MOJAVE	1.08$\pm$0.11
									100 $\pm$ 16	5	MOJAVE	2.15$\pm$0.35
									54 $\pm$ 11	6a	MOJAVE	1.16$\pm$0.24
									330.4 $\pm$ 9.8	8a	MOJAVE	7.08$\pm$0.21
									287 $\pm$ 25	9	MOJAVE	6.14$\pm$0.53
									116 $\pm$ 23	14	MOJAVE	2.48$\pm$0.50
0010+405	F	0.255	8.81	L18					428 $\pm$ 40	1	MOJAVE	6.92$\pm$0.64
									2 $\pm$ 16e	2	MOJAVE	0.04$\pm$0.26
									2.9 $\pm$ 4.3e	3	MOJAVE	0.047$\pm$0.070
									1.1 $\pm$ 3.1e	4	MOJAVE	0.018$\pm$0.050
0014+813	F	3.366	9.31	L18	15.9	0.425	693	0.77	4$\pm$12	C1	B08	0.39$\pm$1.18
									86$\pm$15	C2	B08	8.49$\pm$1.48
									111$\pm$18	C3	B08	10.95$\pm$1.78
0016+731	F	1.781	7.84	L18	18.2	0.735	1136	0.11	106.2 $\pm$ 4.4	1a	MOJAVE	8.23$\pm$0.34
0022+390	F	1.946							113$\pm$43	C1	B08	8.51$\pm$3.24
									71$\pm$57	C2	B08	5.35$\pm$4.29
0026+346	F	0.516597							7 $\pm$ 20	1	MOJAVE	0.22$\pm$0.60
									23 $\pm$ 37	2	MOJAVE	0.7$\pm$1.1
									26 $\pm$ 19	3	MOJAVE	0.81$\pm$0.58
									44 $\pm$ 51	4	MOJAVE	1.3$\pm$1.6
									60 $\pm$ 22	5	MOJAVE	1.85$\pm$0.67
									24 $\pm$ 14	6	MOJAVE	0.73$\pm$0.42
0027+056	F	1.317	0.77	L18	18.9	0.046	294	0.32	22 $\pm$ 46	1	MOJAVE	1.4$\pm$2.9
									67 $\pm$ 53	2	MOJAVE	4.3$\pm$3.4
									22.7 $\pm$ 5.9	3	MOJAVE	1.45$\pm$0.38
0035+367	F	0.366							122$\pm$12	C1	B08	2.58$\pm$0.25
0035+413	F	1.353	14.3	L18	20.3	0.142	692	0.34	83$\pm$17	C1	B08	5$\pm$1.02
									171	C2	B08	10.3$\pm$0
									63$\pm$32	C3	B08	3.8$\pm$1.93
									176$\pm$106	C4	B08	10.6$\pm$6.39
0106+612	G	0.783	23.74	L18	19.4	2.09	305	0.33	372 $\pm$ 180	1	MOJAVE	16.2$\pm$7.8
									468 $\pm$ 30	2	MOJAVE	20.3$\pm$1.3
0108+388	G	0.67	7.42	L18	22	0.109	429	0.03	100		VC94	3.57$\pm$0
0109+351	F	0.45	1.57	L18	18.3	0.125	399	0.63	198 $\pm$ 54	4	MOJAVE	5.4$\pm$1.5
									145 $\pm$ 12	5	MOJAVE	3.92$\pm$0.34
									92 $\pm$ 15	6	MOJAVE	2.50$\pm$0.41
0112-017	F	1.365	14.55	L18	17.8	0.14	1076	0.56	244 $\pm$ 13	2	MOJAVE	15.98$\pm$0.86
									273 $\pm$ 27	3	MOJAVE	17.9$\pm$1.8
0119+115	F	0.57	8.75	L18	19.2	0.073	1184	0.67	48 $\pm$ 13	2	MOJAVE	1.61$\pm$0.45
									557 $\pm$ 25	3	MOJAVE	18.58$\pm$0.82
0122-003	F	1.074	20	L18	16.5	0.074	1540	0.92	213 $\pm$ 74	4	MOJAVE	11.8$\pm$4.1
									169 $\pm$ 10	5	MOJAVE	9.37$\pm$0.56
									120 $\pm$ 37	6	MOJAVE	6.6$\pm$2.0
									164 $\pm$ 22	7	MOJAVE	9.1$\pm$1.2
0133+207	Sy1.5	0.425							240$\pm$50	K	VC94	5.8$\pm$1.21
0136+176	F	2.73	12.43	L18					35 $\pm$ 54	1	MOJAVE	3.4$\pm$5.3
									149 $\pm$ 27	2	MOJAVE	14.6$\pm$2.6
									123 $\pm$ 15	3	MOJAVE	12.0$\pm$1.5
0145+386	F	1.442	9.33	L18	17.4	0.104	345	0	105$\pm$16	C1	B08	6.6$\pm$1.01
0149+218	F	1.32	4.32	L18	18.9	0.171	1042	0.41	20.9 $\pm$ 9.1	1	MOJAVE	1.34$\pm$0.58
									223 $\pm$ 12	2a	MOJAVE	14.29$\pm$0.76
									122.4 $\pm$ 9.4	4	MOJAVE	7.83$\pm$0.60
									6.3 $\pm$ 1.7e	7	MOJAVE	0.41$\pm$0.11
0151+474	F	1.026	34.72	L18	19	0.319	275	0	23$\pm$52	C1	B08	1.14$\pm$2.58
									87$\pm$18	C2	B08	4.32$\pm$0.89
0153+744	F	2.338			16.7	1.116	1801	0.22	66	C1	B08	5.49$\pm$0
									25$\pm$154	C2	B08	2.08$\pm$12.8
									463$\pm$290	C3	B08	38.5$\pm$24.11
									698$\pm$189	C4	B08	58.04$\pm$15.71
									173$\pm$89	C5	B08	14.38$\pm$7.4
									22$\pm$27	C6	B08	1.83$\pm$2.24
0208?512	F	1.003			14.8	0.047	3493	0.75	600		SHW98	29.33$\pm$0
0224+671	F	0.53	6.01	L18	18.1	2.274	1540	0.39	258.6 $\pm$ 8.1	1	MOJAVE	8.01$\pm$0.25
									20 $\pm$ 10e	3	MOJAVE	0.61$\pm$0.31
									140.6 $\pm$ 6.7	4a	MOJAVE	4.35$\pm$0.21
									373.6 $\pm$ 6.8	5a	MOJAVE	11.56$\pm$0.21
									290 $\pm$ 11	8a	MOJAVE	8.98$\pm$0.33
									356 $\pm$ 17	12	MOJAVE	11.01$\pm$0.51
0229+131	F	2.059	11.31	L18	17.5	0.278	1560	0.35	40 $\pm$ 31	1	MOJAVE	3.4$\pm$2.6
									166 $\pm$ 15	3	MOJAVE	14.0$\pm$1.2
									84.4 $\pm$ 6.8	4	MOJAVE	7.11$\pm$0.57
0241+622	G	0.044	1.71	L18					513 $\pm$ 15	2a	MOJAVE	1.526$\pm$0.044
									230.7 $\pm$ 6.4	4	MOJAVE	0.687$\pm$0.019
0248+430	F	1.31	17.42	L18	17.1	0.246	1225	0.29	102 $\pm$ 12	1	MOJAVE	6.49$\pm$0.73
									91.4 $\pm$ 5.6	3	MOJAVE	5.82$\pm$0.36
									95.7 $\pm$ 8.7	4	MOJAVE	6.09$\pm$0.56
0355+508	F	1.52	6.12	L18	18.1	3.427	4297	0.78	21 $\pm$ 16	1	MOJAVE	1.5$\pm$1.1
									8 $\pm$ 13	2	MOJAVE	0.53$\pm$0.93
0400+258	F	2.109	7.59	L18	19.6	0.461	936	0.14	16 $\pm$ 73	1	MOJAVE	1.4$\pm$6.3
									94 $\pm$ 102	2	MOJAVE	8.1$\pm$8.7
									72 $\pm$ 107	3	MOJAVE	6.1$\pm$9.1
									137.4 $\pm$ 9.4	4	MOJAVE	11.74$\pm$0.80
0429+415	G	1.023							58 $\pm$ 17	1	MOJAVE	3.10$\pm$0.89
									25.5 $\pm$ 8.5	2	MOJAVE	1.36$\pm$0.45
									14 $\pm$ 22	3	MOJAVE	0.7$\pm$1.2
									19.0 $\pm$ 9.0	5	MOJAVE	1.01$\pm$0.48
									7.1 $\pm$ 4.1	6	MOJAVE	0.38$\pm$0.22
									13.7 $\pm$ 7.7	7	MOJAVE	0.73$\pm$0.41
0430+052	F	0.033	1.09	L18	13.8	0.68	3440	22.7	2187 $\pm$ 93	1a	MOJAVE	4.80$\pm$0.20
									1724 $\pm$ 20	2a	MOJAVE	3.783$\pm$0.043
									2308 $\pm$ 27	3	MOJAVE	5.065$\pm$0.059
									1940 $\pm$ 91	4	MOJAVE	4.26$\pm$0.20
									1772 $\pm$ 45	5a	MOJAVE	3.889$\pm$0.099
									1939 $\pm$ 70	6	MOJAVE	4.26$\pm$0.15
									2091 $\pm$ 38	7	MOJAVE	4.590$\pm$0.083
									1506 $\pm$ 46	8	MOJAVE	3.31$\pm$0.10
									2295 $\pm$ 25	11a	MOJAVE	5.038$\pm$0.055
									2224 $\pm$ 69	12	MOJAVE	4.88$\pm$0.15
									2649 $\pm$ 21	13a	MOJAVE	5.814$\pm$0.047
									2941 $\pm$ 109	14a	MOJAVE	6.46$\pm$0.24
									2402 $\pm$ 87	15	MOJAVE	5.27$\pm$0.19
									1904 $\pm$ 39	24	MOJAVE	4.180$\pm$0.085
									1943 $\pm$ 59	29	MOJAVE	4.26$\pm$0.13
									2404 $\pm$ 50	30	MOJAVE	5.28$\pm$0.11
									2870 $\pm$ 20	31a	MOJAVE	6.299$\pm$0.044
									2736 $\pm$ 28	32a	MOJAVE	6.006$\pm$0.061
									1690 $\pm$ 109	33	MOJAVE	3.71$\pm$0.24
									2117 $\pm$ 99	35	MOJAVE	4.65$\pm$0.22
									2170 $\pm$ 22	36a	MOJAVE	4.762$\pm$0.048
									1831 $\pm$ 132	37	MOJAVE	4.02$\pm$0.29
									2457 $\pm$ 46	38a	MOJAVE	5.39$\pm$0.10
									2209 $\pm$ 74	41a	MOJAVE	4.85$\pm$0.16
									2393 $\pm$ 108	43	MOJAVE	5.25$\pm$0.24
									2323 $\pm$ 122	44	MOJAVE	5.10$\pm$0.27
0454+844	F	1.34			17.4	0.24	295	0.39	45 $\pm$ 10	2	MOJAVE	2.70$\pm$0.60
									107 $\pm$ 21	3	MOJAVE	6.41$\pm$1.26
									13.2 $\pm$ 2.2	5	MOJAVE	0.79$\pm$0.13
0536+145	F	2.69	22.59	L18	19.8	1.146	433	0	234 $\pm$ 118	1	MOJAVE	20.88$\pm$10.53
									127 $\pm$ 43	2	MOJAVE	11.33$\pm$3.84
0552+398	F	2.365	25.2	H09	18.1	1.023	1517	0.65	234 $\pm$ 118	1	MOJAVE	23$\pm$11
									127 $\pm$ 43	2	MOJAVE	12.3$\pm$4.2
0607-157	F	0.323	14.25	L18	15.3	0.602	2742	0.87	40 $\pm$ 17	1	MOJAVE	0.80$\pm$0.35
									60 $\pm$ 41	2	MOJAVE	1.20$\pm$0.83
									28.3 $\pm$ 9.1	3	MOJAVE	0.57$\pm$0.18
0615+820	F	0.71	8.06	L18					50$\pm$50		VC94	1.87$\pm$1.87
0642+449	F	3.396	10.7	H09	18.3	0.251	452	0.39	12.6 $\pm$ 1.3	1	MOJAVE	1.36$\pm$0.14
									78.9 $\pm$ 3.8	3	MOJAVE	8.52$\pm$0.41
									32.8 $\pm$ 4.8	4	MOJAVE	3.54$\pm$0.52
0646+600	F	0.455	3.27	L18	19.8	0.16	472	0	39 $\pm$ 16	1	MOJAVE	1.08$\pm$0.44
									31 $\pm$ 16	2	MOJAVE	0.85$\pm$0.43
									38 $\pm$ 13	3	MOJAVE	1.05$\pm$0.36
									9.64 $\pm$ 0.73	4	MOJAVE	0.264$\pm$0.020
									2.63 $\pm$ 0.95	5	MOJAVE	0.072$\pm$0.026
									12.8 $\pm$ 2.8	8	MOJAVE	0.352$\pm$0.077
0723+679	S1.2	0.846							190		VC94	8.17$\pm$0
0738+313	F	0.63	7.35	L18	16.8	0.105	2284	0.54	295 $\pm$ 34	1	MOJAVE	10.7$\pm$1.2
									255 $\pm$ 12	2	MOJAVE	9.25$\pm$0.42
									164.6 $\pm$ 3.7	3	MOJAVE	5.98$\pm$0.13
									112.2 $\pm$ 4.3	4a	MOJAVE	4.08$\pm$0.16
									88.8 $\pm$ 3.1	6a	MOJAVE	3.23$\pm$0.11
									160.8 $\pm$ 4.3	8a	MOJAVE	5.84$\pm$0.16
0743-006	F	0.994	4.7	L18	17.2	0.097	661	0.78	42.2 $\pm$ 7.7	1	MOJAVE	2.20$\pm$0.40
									16.3 $\pm$ 7.5	2	MOJAVE	0.85$\pm$0.39
									49 $\pm$ 10	3	MOJAVE	2.56$\pm$0.52
0745+241	F	0.409	1.81	L18	18.6	0.126	958	1.24	265 $\pm$ 29	3	MOJAVE	6.60$\pm$0.72
									14.8 $\pm$ 5.7e	9	MOJAVE	0.37$\pm$0.14
									14.1 $\pm$ 4.6e	11	MOJAVE	0.35$\pm$0.11
									6.6 $\pm$ 2.0e	12	MOJAVE	0.165$\pm$0.049
									3.98 $\pm$ 1.00e	13	MOJAVE	0.099$\pm$0.025
									62 $\pm$ 30	14	MOJAVE	1.55$\pm$0.75
									35 $\pm$ 40	15	MOJAVE	0.9$\pm$1.0
0804+499	F	1.435	8.63	L18	18.6	0.121	1115	0.27	74$\pm$33	C1	CJF	4.63$\pm$2.07
									269$\pm$58	C2	CJF	16.84$\pm$3.63
0834-201	F	2.752			18.5	0.23	1971	0.47	22 $\pm$ 11	1	MOJAVE	2.2$\pm$1.1
									70.7 $\pm$ 8.4	3	MOJAVE	6.93$\pm$0.82
0839+616	F	0.862							230$\pm$50		VC94	10.03$\pm$2.18
0846+513	F	0.585	22.77	L18	18.3	0.059	266	0.12	52 $\pm$ 43	4	MOJAVE	1.8$\pm$1.5
									172 $\pm$ 26	5	MOJAVE	5.84$\pm$0.89
									136 $\pm$ 41	6	MOJAVE	4.6$\pm$1.4
0847-120			16.5	H09					194 $\pm$ 47	1	MOJAVE	6.4$\pm$1.6
									92 $\pm$ 14	3	MOJAVE	3.06$\pm$0.45
0850+581	F	1.322	11.26	L18	17.7	0.127	1102	0.26	118.3 $\pm$ 5.9	1	MOJAVE	7.56$\pm$0.38
									94 $\pm$ 18	2	MOJAVE	6.0$\pm$1.2
									109.9 $\pm$ 5.9	3	MOJAVE	7.02$\pm$0.38
									82.3 $\pm$ 7.0	4	MOJAVE	5.26$\pm$0.45
									87 $\pm$ 17	5	MOJAVE	5.6$\pm$1.1
									79.5 $\pm$ 8.1	6	MOJAVE	5.08$\pm$0.52
									76.4 $\pm$ 1.5	7	MOJAVE	4.882$\pm$0.099
									49.8 $\pm$ 1.0	8	MOJAVE	3.182$\pm$0.067
0859-140	F	1.332	3.34	L18	16.4	0.14	2898	0.65	116 $\pm$ 21	1	MOJAVE	7.5$\pm$1.4
									78 $\pm$ 11	2	MOJAVE	5.04$\pm$0.73
									76.4 $\pm$ 3.6	3	MOJAVE	4.93$\pm$0.23
									114 $\pm$ 56	4	MOJAVE	7.4$\pm$3.6
									5.7 $\pm$ 6.5e	5	MOJAVE	0.37$\pm$0.42
									56.3 $\pm$ 4.9	6	MOJAVE	3.64$\pm$0.32
									39 $\pm$ 11	7	MOJAVE	2.52$\pm$0.72
0906+430	HP AGN	0.67			18.8	0.043	4234	0.4	13	A	VC94	0.46$\pm$0
									180$\pm$30	B	VC94	6.42$\pm$1.07
0923+392	F	0.698	3.16	L18	16.6	0.034	2885	2.13	39.5 $\pm$ 1.1	2	MOJAVE	1.557$\pm$0.045
									70 $\pm$ 14	7	MOJAVE	2.75$\pm$0.54
									33.5 $\pm$ 6.0	8	MOJAVE	1.32$\pm$0.24
									8.0 $\pm$ 2.0	9	MOJAVE	0.316$\pm$0.077
									56.8 $\pm$ 3.0	19a	MOJAVE	2.24$\pm$0.12
0955+476	F	1.882	12.01	L18	18.5	0.033	604	0.46	3.5 $\pm$ 5.7e	1	MOJAVE	0.28$\pm$0.46
									22.5 $\pm$ 3.8	2	MOJAVE	1.81$\pm$0.31
									90.4 $\pm$ 9.2	5	MOJAVE	7.24$\pm$0.74
									28.7 $\pm$ 7.3	7	MOJAVE	2.30$\pm$0.59
1012+232	F	0.565	6.68	L18	17.5	0.058	1096	0.54	289 $\pm$ 17	2	MOJAVE	9.57$\pm$0.56
									246 $\pm$ 25	3	MOJAVE	8.13$\pm$0.83
1023+259	F	5.28							26$\pm$31	B	Frey2014	3.04$\pm$3.63
									86$\pm$33	C	Frey2014	10.06$\pm$3.86
									112$\pm$31	D	Frey2014	13.1$\pm$3.63
									100$\pm$31	E	Frey2014	11.7$\pm$3.63
1034-293	F	0.312	2.8	F09	17.5	0.118	1113	0.83	334 $\pm$ 36	4	MOJAVE	6.49$\pm$0.69
1036+054	F	0.473	7.92	L18	19.1	0.059	640	0.35	223 $\pm$ 45	1	MOJAVE	6.3$\pm$1.3
									196 $\pm$ 12	2a	MOJAVE	5.57$\pm$0.34
1038+528	F	2.296	4	F09	16.7	0.031	698	0.6	140	C1	Marc85	11.53$\pm$0
									180	C2	Marc85	14.83$\pm$0
1040+123	F	1.028	3.4	F09					110$\pm$50	A2	VC94	5.47$\pm$2.49
1045-188	F	0.595	12.47	L18	18	0.088	1156	0.69	9 $\pm$ 18e	1	MOJAVE	0.31$\pm$0.63
									299.4 $\pm$ 9.1	3	MOJAVE	10.35$\pm$0.32
1049+215	F	1.3	6.29	L18	18.4	0.057	1254	0.32	99.3 $\pm$ 8.6	1	MOJAVE	6.29$\pm$0.54
									22 $\pm$ 35	2	MOJAVE	1.4$\pm$2.2
									54 $\pm$ 11	3	MOJAVE	3.42$\pm$0.72
1055+201	F	1.11	1.33	L18	16.9	0.055	2143	1.21	127 $\pm$ 26	1	MOJAVE	7.2$\pm$1.5
									97 $\pm$ 19	2	MOJAVE	5.5$\pm$1.1
									131 $\pm$ 17	3	MOJAVE	7.45$\pm$0.98
1128+385	F	1.74			18.7	0.058	702	0.4	39.0 $\pm$ 8.7	1	MOJAVE	2.97$\pm$0.66
									21.8 $\pm$ 7.8	2	MOJAVE	1.66$\pm$0.60
									38 $\pm$ 20	3	MOJAVE	2.9$\pm$1.5
									43.3 $\pm$ 3.7	4	MOJAVE	3.30$\pm$0.28
1128-047	G	0.266	0.51	L18	18.7	0.118	561	0.16	260 $\pm$ 191	1	MOJAVE	4.4$\pm$3.2
									184 $\pm$ 91	2	MOJAVE	3.1$\pm$1.5
									123 $\pm$ 52	3	MOJAVE	2.06$\pm$0.87
									69 $\pm$ 14	4	MOJAVE	1.15$\pm$0.23
									15.4 $\pm$ 8.3	5	MOJAVE	0.26$\pm$0.14
									57.4 $\pm$ 9.3	6	MOJAVE	0.96$\pm$0.16
1137+660	Sy 1.2	0.646	1.42	F09					60$\pm$20		VC94	2.08$\pm$0.69
1144+35	F	0.063							490$\pm$18	C1	Gio99a	1.92$\pm$0.07
									460$\pm$18	C2	Gio99a	1.81$\pm$0.07
1148-001	F	1.98			17	0.053	2774	0.55	92.0 $\pm$ 5.4	3a	MOJAVE	7.58$\pm$0.45
									51 $\pm$ 12	5	MOJAVE	4.24$\pm$0.97
									78.2 $\pm$ 3.7	6	MOJAVE	6.45$\pm$0.30
									120 $\pm$ 14	7	MOJAVE	9.9$\pm$1.1
1150+497	F/QSO	0.334	7.81	L18	17	0.052	110	0.28	845 $\pm$ 98	1	MOJAVE	17.5$\pm$2.0
									477 $\pm$ 20	2	MOJAVE	9.86$\pm$0.41
									392 $\pm$ 20	5	MOJAVE	8.11$\pm$0.41
									398 $\pm$ 39	7	MOJAVE	8.23$\pm$0.80
									290 $\pm$ 21	8	MOJAVE	6.00$\pm$0.43
									304 $\pm$ 17	11	MOJAVE	6.27$\pm$0.34
1150+812	F	1.25	3.2	L18	18.4	0.175	1343	0.36	119.7 $\pm$ 5.7	2	MOJAVE	7.38$\pm$0.35
									109.5 $\pm$ 3.7	3a	MOJAVE	6.75$\pm$0.23
									164.4 $\pm$ 8.6	4a	MOJAVE	10.13$\pm$0.53
									100.0 $\pm$ 9.6	5	MOJAVE	6.17$\pm$0.59
									109.0 $\pm$ 3.7	6a	MOJAVE	6.72$\pm$0.23
									114 $\pm$ 16	7	MOJAVE	7.00$\pm$1.00
1157-215	F	0.927			17.8	0.104	386	0	9.3 $\pm$ 3.8	1	MOJAVE	0.46$\pm$0.19
									83 $\pm$ 22	2	MOJAVE	4.1$\pm$1.1
									26.2 $\pm$ 8.0	3	MOJAVE	1.30$\pm$0.40
1302-102	F	0.278	10.03	L18	14.4	0.099	711	4.02	177 $\pm$ 22	3	MOJAVE	3.09$\pm$0.38
									487 $\pm$ 16	4a	MOJAVE	8.50$\pm$0.28
									399 $\pm$ 34	5	MOJAVE	6.96$\pm$0.59
									433 $\pm$ 33	6	MOJAVE	7.56$\pm$0.58
									380 $\pm$ 53	8	MOJAVE	6.64$\pm$0.92
1331+170	F	2.084	1.98	L18	16.1	0.051	391	0.64	63.7 $\pm$ 6.0	1	MOJAVE	5.40$\pm$0.51
									47.1 $\pm$ 3.5	2	MOJAVE	3.99$\pm$0.30
1435+638	F	2.068	0.83	L18	17	0.036	952	0.34	66 $\pm$ 16	1	MOJAVE	5.6$\pm$1.4
									93.7 $\pm$ 2.2	3	MOJAVE	7.92$\pm$0.19
									15.7 $\pm$ 7.5	5	MOJAVE	1.33$\pm$0.63
									28.8 $\pm$ 2.9	6	MOJAVE	2.44$\pm$0.24
									6.2 $\pm$ 5.0e	7	MOJAVE	0.52$\pm$0.42
1458+718	Sy 1.5	0.905	3.92	L18	17.2	0.056	7468	0.77	65 $\pm$ 29	1	MOJAVE	3.2$\pm$1.4
									83 $\pm$ 19	2a	MOJAVE	4.03$\pm$0.92
									55 $\pm$ 11	3	MOJAVE	2.66$\pm$0.55
									28.3 $\pm$ 5.7	4	MOJAVE	1.37$\pm$0.28
									14.7 $\pm$ 8.8	5	MOJAVE	0.71$\pm$0.43
									138.4 $\pm$ 5.6	6	MOJAVE	6.72$\pm$0.27
									117.1 $\pm$ 4.3	7a	MOJAVE	5.69$\pm$0.21
1504?166	F	0.876	18.41	L18	18.8	0.215	2711	6.11	75.0 $\pm$ 7.1	1a	MOJAVE	3.56$\pm$0.34
									35.4 $\pm$ 6.4	2	MOJAVE	1.68$\pm$0.30
									83.6 $\pm$ 1.9	3a	MOJAVE	3.966$\pm$0.089
									97.3 $\pm$ 4.3	5	MOJAVE	4.61$\pm$0.20
1532+016	F	1.42	10.13	L18	19.3	0.117	1344	0.9	13.2 $\pm$ 4.6	1	MOJAVE	0.89$\pm$0.31
									97.1 $\pm$ 9.7	2	MOJAVE	6.57$\pm$0.65
									99.8 $\pm$ 6.9	4	MOJAVE	6.75$\pm$0.46
1617+229	F	1.987	9.37	L18	19.9	0.158	475	0	41 $\pm$ 49	1	MOJAVE	3.4$\pm$4.1
									26.8 $\pm$ 8.7	2	MOJAVE	2.22$\pm$0.72
									48.8 $\pm$ 3.2	3	MOJAVE	4.03$\pm$0.26
									18 $\pm$ 16	4	MOJAVE	1.5$\pm$1.4
1618+177	Sy 1.5	0.555							100$\pm$30		VC94	3.05$\pm$0.91
1637+574	F	0.75	7.97	L18	16.8	0.027	1199	1.04	213.0 $\pm$ 9.7	1a	MOJAVE	8.94$\pm$0.40
									306 $\pm$ 16	2	MOJAVE	12.84$\pm$0.69
									181 $\pm$ 18	5	MOJAVE	7.60$\pm$0.74
									228 $\pm$ 16	6a	MOJAVE	9.56$\pm$0.67
									280 $\pm$ 16	7	MOJAVE	11.76$\pm$0.68
									324 $\pm$ 21	9	MOJAVE	13.61$\pm$0.89
1642+690	F	0.751	3.12	L18	18.6	0.086	1720	0.32	32.2 $\pm$ 6.7	1	MOJAVE	1.35$\pm$0.28
									346.4 $\pm$ 6.2	3a	MOJAVE	14.54$\pm$0.26
									78 $\pm$ 11	5	MOJAVE	3.26$\pm$0.47
									25 $\pm$ 11	9	MOJAVE	1.06$\pm$0.46
									235 $\pm$ 18	10	MOJAVE	9.86$\pm$0.77
1655+077	F	0.621	6.24	L18	19.5	0.344	1413	0.56	156 $\pm$ 29	1	MOJAVE	5.6$\pm$1.0
									22.5 $\pm$ 7.2	2	MOJAVE	0.81$\pm$0.26
									412 $\pm$ 31	5	MOJAVE	14.8$\pm$1.1
									310 $\pm$ 11	6	MOJAVE	11.13$\pm$0.38
									273 $\pm$ 15	7	MOJAVE	9.79$\pm$0.54
									301.8 $\pm$ 9.8	9a	MOJAVE	10.82$\pm$0.35
									95.1 $\pm$ 8.7	10	MOJAVE	3.41$\pm$0.31
1721+343	F	0.206							160$\pm$50	B	VC94	1.98$\pm$0.62
									280$\pm$30	C	VC94	3.47$\pm$0.37
1751+288	F	1.115	3.81	L18	20.3	0.136	414	0.28	70.8 $\pm$ 6.4	1	MOJAVE	4.03$\pm$0.36
1758+388	F	2.092	3.62	L18	17.5	0.062	326	0.68	26.0 $\pm$ 2.1	3	MOJAVE	2.22$\pm$0.18
									15.0 $\pm$ 1.3	4	MOJAVE	1.28$\pm$0.11
1845+797	F	0.057	0.91	L18					589 $\pm$ 13	1	MOJAVE	2.157$\pm$0.049
									544 $\pm$ 12	3a	MOJAVE	1.993$\pm$0.042
									284 $\pm$ 44	4	MOJAVE	1.04$\pm$0.16
									427 $\pm$ 37	5	MOJAVE	1.56$\pm$0.14
									265 $\pm$ 35	10	MOJAVE	0.97$\pm$0.13
1901+319	Sy 1.5	0.635			15.8	0.275	3204	0.53	15.2 $\pm$ 1.7e	1	MOJAVE	0.555$\pm$0.063
									241.1 $\pm$ 6.6	2	MOJAVE	8.81$\pm$0.24
									213.5 $\pm$ 5.8	4	MOJAVE	7.80$\pm$0.21
									86.6 $\pm$ 4.9	5a	MOJAVE	3.16$\pm$0.18
									181 $\pm$ 11	7	MOJAVE	6.61$\pm$0.40
									193 $\pm$ 13	9	MOJAVE	7.05$\pm$0.49
									181 $\pm$ 18	11	MOJAVE	6.62$\pm$0.67
									75 $\pm$ 35	12	MOJAVE	2.7$\pm$1.3
1928+738	F	0.302	4.96	L18	15.2	0.307	3950	3.66	433 $\pm$ 11	1	MOJAVE	8.16$\pm$0.21
									400 $\pm$ 56	2	MOJAVE	7.5$\pm$1.1
									259.8 $\pm$ 8.3	3a	MOJAVE	4.90$\pm$0.16
									349 $\pm$ 14	4	MOJAVE	6.58$\pm$0.26
									268.7 $\pm$ 8.1	5	MOJAVE	5.07$\pm$0.15
									254.6 $\pm$ 3.8	6a	MOJAVE	4.803$\pm$0.071
									259.6 $\pm$ 3.5	8a	MOJAVE	4.898$\pm$0.066
									244.2 $\pm$ 7.7	9	MOJAVE	4.61$\pm$0.15
									254.7 $\pm$ 4.9	10a	MOJAVE	4.805$\pm$0.092
									159.9 $\pm$ 3.6	11a	MOJAVE	3.017$\pm$0.068
									158 $\pm$ 17	12	MOJAVE	2.99$\pm$0.33
									134 $\pm$ 11	13	MOJAVE	2.53$\pm$0.21
									30 $\pm$ 18	15	MOJAVE	0.56$\pm$0.34
1936-155	F	1.657	48.29	L18	20.6	0.372	609	0.45	20 $\pm$ 14	1	MOJAVE	1.5$\pm$1.0
									72.5 $\pm$ 7.9	2	MOJAVE	5.37$\pm$0.58
									28.0 $\pm$ 5.9	5	MOJAVE	2.08$\pm$0.44
1951+498	F	0.466							28.9 $\pm$ 7.9	3a	MOJAVE	2.21$\pm$0.60
2005+403	F	1.736	41.26	L18	20.3	1.582	2470	0.73	130 $\pm$ 16	4	MOJAVE	9.9$\pm$1.2
									40 $\pm$ 21	10	MOJAVE	3.0$\pm$1.6
2008-159	F	1.18	7.75	L18	16.8	0.336	547	1.72	90 $\pm$ 10	1a	MOJAVE	5.30$\pm$0.59
2037+511	F	1.686	19.86	L18	18.9	2.392	6081	0.28	90 $\pm$ 19	1	MOJAVE	6.7$\pm$1.4
									21.7 $\pm$ 4.6	2a	MOJAVE	1.63$\pm$0.35
									7 $\pm$ 28e	3	MOJAVE	0.5$\pm$2.1
									64.4 $\pm$ 5.9	6	MOJAVE	4.83$\pm$0.45
2121+053	F	1.941	10.31	L18	17.4	0.167	794	0.35	142.7 $\pm$ 9.0	2a	MOJAVE	11.64$\pm$0.74
									88.9 $\pm$ 6.5	3	MOJAVE	7.25$\pm$0.53
2126-158	F	3.268	6.36	L18	16.5	0.18	590	1.54	37.2 $\pm$ 4.2	2	MOJAVE	3.96$\pm$0.45
2128-123	F	0.501	21.36	L18	15.3	0.147	1770	2.82	208.7 $\pm$ 8.3	3a	MOJAVE	6.22$\pm$0.25
									207 $\pm$ 11	4	MOJAVE	6.17$\pm$0.33
									33.2 $\pm$ 7.0	6	MOJAVE	0.99$\pm$0.21
									19.0 $\pm$ 4.3e	7	MOJAVE	0.57$\pm$0.13
									26.5 $\pm$ 3.2	8	MOJAVE	0.790$\pm$0.096
									12.0 $\pm$ 2.8e	9	MOJAVE	0.358$\pm$0.083
									239 $\pm$ 10	12	MOJAVE	7.12$\pm$0.31
									190.2 $\pm$ 9.0	13	MOJAVE	5.67$\pm$0.27
2134+004	F	1.945	1.71	L18	16.8	0.152	3473	0.98	1.7 $\pm$ 3.1e	1	MOJAVE	0.14$\pm$0.25
									62.3 $\pm$ 4.0	2a	MOJAVE	5.07$\pm$0.32
									24.8 $\pm$ 2.5	4	MOJAVE	2.02$\pm$0.20
									15.9 $\pm$ 2.8	5a	MOJAVE	1.29$\pm$0.23
2136+141	F	2.427	4.48	L18	18.2	0.227	1132	0.46	29 $\pm$ 10	1	MOJAVE	2.68$\pm$0.97
									28.0 $\pm$ 6.4	2	MOJAVE	2.58$\pm$0.59
									44.9 $\pm$ 2.0	3a	MOJAVE	4.13$\pm$0.18
									33.8 $\pm$ 1.3	4a	MOJAVE	3.11$\pm$0.12
									22.1 $\pm$ 1.5	5a	MOJAVE	2.03$\pm$0.14
2201+315	F	0.298	2.95	L18	14.3	0.281	2878	3.22	324.5 $\pm$ 6.6	1	MOJAVE	5.98$\pm$0.12
									338.1 $\pm$ 6.9	2a	MOJAVE	6.23$\pm$0.13
									10.0 $\pm$ 4.6e	3	MOJAVE	0.185$\pm$0.084
									377 $\pm$ 11	4	MOJAVE	6.95$\pm$0.20
									332 $\pm$ 14	5	MOJAVE	6.12$\pm$0.26
									449.1 $\pm$ 5.3	6a	MOJAVE	8.281$\pm$0.097
									433 $\pm$ 26	7	MOJAVE	7.98$\pm$0.48
									250 $\pm$ 21	8	MOJAVE	4.61$\pm$0.38
2216-038	F	0.901	12.23	L18	16.3	0.226	2218	0.75	117.8 $\pm$ 5.4	1a	MOJAVE	5.71$\pm$0.26
									139 $\pm$ 14	2	MOJAVE	6.75$\pm$0.70
									118.2 $\pm$ 7.7	3	MOJAVE	5.73$\pm$0.37
2223+210	F	1.959	11.26	L18	17.8	0.107	1838	1.54	203.6 $\pm$ 9.9	1	MOJAVE	16.69$\pm$0.81
									361 $\pm$ 26	2	MOJAVE	29.6$\pm$2.2
									142 $\pm$ 28	3	MOJAVE	11.7$\pm$2.3
2243-123	F	0.63	9.03	L18	16.8	0.117	1882	1.43	58 $\pm$ 13	1	MOJAVE	2.11$\pm$0.49
									135.7 $\pm$ 5.9	2	MOJAVE	4.94$\pm$0.22
									119.8 $\pm$ 7.1	3a	MOJAVE	4.36$\pm$0.26
2318+049	F	0.622			18.5	0.148	542	0.59	177 $\pm$ 17	1	MOJAVE	6.37$\pm$0.61
									155 $\pm$ 16	3	MOJAVE	5.58$\pm$0.59
2351+456	F	1.992	3.36	L18	19.1	0.286	1872	0.26	266 $\pm$ 17	1	MOJAVE	22.0$\pm$1.4
									19.4 $\pm$ 7.8e	2	MOJAVE	1.61$\pm$0.65
									185 $\pm$ 13	4	MOJAVE	15.3$\pm$1.0
									133.8 $\pm$ 7.5	5	MOJAVE	11.05$\pm$0.62
									234 $\pm$ 11	6	MOJAVE	19.32$\pm$0.91
									304 $\pm$ 21	7	MOJAVE	25.1$\pm$1.7
2356+196	F	1.066	3.2	L18	17.8	0.126	673	0.31	14.5 $\pm$ 3.0	1	MOJAVE	0.80$\pm$0.17
									14 $\pm$ 12	2	MOJAVE	0.78$\pm$0.65
									19 $\pm$ 12	3	MOJAVE	1.03$\pm$0.65
									20 $\pm$ 11	4	MOJAVE	1.09$\pm$0.58
									13.0 $\pm$ 7.7	5a	MOJAVE	0.72$\pm$0.43
									28.6 $\pm$ 5.0	6	MOJAVE	1.57$\pm$0.27

Equations

$$\delta \ge [1.54\times 10^{-3}(1+z{)}^{4+2\alpha }(\frac{d_{\mathrm{L}}}{\mathrm{Mpc}}{)}^2(\frac{\Delta T}{\mathrm{hr}}{)}^{-1}(\frac{F_{1KeV}}{\mu \mathrm{Jy}})(\frac{E_{\gamma }}{\mathrm{GeV}}{)}^{\alpha }{]}^{\frac{1}{4+2\alpha }}$$

$${\beta }_{\mathrm{app}}=\frac{\mu }{H_0}{\int }_1^{1+z}\frac{1}{\sqrt{{\Omega }_{\mathrm{M}}{x}^3+1-{\Omega }_{\mathrm{M}}}}dx.$$

$$\sigma =\sqrt{\sum _{i=1}^n(\frac{\partial f}{\partial x_i}{)}^2{\sigma }_{x_i}^2}$$

$$\log {\mu }_{\mathrm{FDS}}^{\max }=-(0.35\pm 0.10)\log z-(0.95\pm 0.03)$$

$$\log {\mu }_{\mathrm{non}-\mathrm{FDS}}^{\max }=-(0.14\pm 0.11)\log z-(0.96\pm 0.04)$$

$$\log {\beta }_{\mathrm{FDS}}^{\max }=(0.36\pm 0.09)\log z+(0.76\pm 0.03),r=0.28\mathrm{and}p=1.4\times 10^{-4},\mathrm{and}$$

$$\log {\beta }_{\mathrm{FDS}}^{\mathrm{mean}}=(0.30\pm 0.09)\log z+(0.55\pm 0.03),r=0.24\mathrm{and}p=1.0\times 10^{-3},$$

$$\log {\beta }_{\mathrm{non}-\mathrm{FDS}}^{\max }=(0.59\pm 0.10)\log z+(0.73\pm 0.03),r=0.50\mathrm{and}p=1.6\times 10^{-7},\mathrm{and}$$

$$\log {\beta }_{\mathrm{non}-\mathrm{FDS}}^{\mathrm{mean}}=(0.54\pm 0.11)\log z+(0.55\pm 0.03),r=0.46\mathrm{and}p=2.8\times 10^{-6},$$

$$f=N_{(E_{\mathrm{L}}\sim E_{\mathrm{U}})}(\frac{1}{E_{\mathrm{L}}}-\frac{1}{E_{\mathrm{U}}})\ln \frac{E_{\mathrm{U}}}{E_{\mathrm{L}}},\mathrm{if}{\alpha }_{\mathrm{ph}}=2,\mathrm{otherwise}$$

$$f=N_{(E_{\mathrm{L}}\sim E_{\mathrm{U}})}\frac{1-{\alpha }_{\mathrm{ph}}}{2-{\alpha }_{\mathrm{ph}}}\frac{(E_{\mathrm{U}}^{2-{\alpha }_{\mathrm{ph}}}-E_{\mathrm{L}}^{2-{\alpha }_{\mathrm{ph}}})}{(E_{\mathrm{U}}^{1-{\alpha }_{\mathrm{ph}}}-E_{\mathrm{L}}^{1-{\alpha }_{\mathrm{ph}}})}$$

$$L_{\gamma }=4\pi d_{\mathrm{L}}^2(1+z{)}^{{\alpha }_{\mathrm{ph}}-2}f$$

$$\log S_{\mathrm{r}}=(0.28\pm 0.04)\log F_{\mathrm{o}}+(6.15\pm 0.49),r=0.51\mathrm{and}p=5.9\times 10^{-14},$$

$$\log F_{\mathrm{x}}=(0.46\pm 0.04)\log F_{\mathrm{o}}+(5.46\pm 0.51),r=0.64\mathrm{and}p=6.8\times 10^{-22},\mathrm{and}$$

$$\log F_{\mathrm{x}}=(0.53\pm 0.08)\log S_{\mathrm{r}}-(1.65\pm 0.22),r=0.46\mathrm{and}p=1.0\times 10^{-10}$$

$$\log S_{\mathrm{r}}=(0.28\pm 0.07)\log F_{\mathrm{o}}+(6.21\pm 0.82),r=0.38\mathrm{and}p=4.0\times 10^{-4},$$

$$\log F_{\mathrm{x}}=(0.40\pm 0.06)\log F_{\mathrm{o}}+(4.63\pm 0.78),r=0.47\mathrm{and}p=1.8\times 10^{-5},\mathrm{and}$$

$$\log F_{\mathrm{x}}=(0.51\pm 0.11)\log S_{\mathrm{r}}-(1.70\pm 0.30),r=0.50\mathrm{and}p=3.7\times 10^{-6}$$

$$\log S_{\mathrm{r}}=(0.13\pm 0.06)\log F_{\mathrm{o}}+(4.37\pm 0.71),r=0.37\mathrm{and}p=1.2\%,$$

$$\log F_{\mathrm{X}}=(0.58\pm 0.09)\log F_{\mathrm{o}}+(7.10\pm 1.06),r=0.80\mathrm{and}p=3.1\times 10^{-7},and$$

$$\log F_{\mathrm{X}}=(0.68\pm 0.23)\log S_{\mathrm{r}}-(1.87\pm 0.69),r=0.36\mathrm{and}p=1.7\%.$$

$$\log S_{\mathrm{r}}=(0.16\pm 0.04)\log F_{\mathrm{o}}+(4.86\pm 0.47),r=0.34\mathrm{and}p=1.5\times 10^{-7},$$

$$\log F_{\mathrm{X}}=(0.47\pm 0.04)\log F_{\mathrm{o}}+(5.61\pm 0.47),r=0.60\mathrm{and}p=9.6\times 10^{-23},$$

$$\log F_{\mathrm{X}}=(0.42\pm 0.07)\log S_{\mathrm{r}}-(1.41\pm 0.23),r=0.36\mathrm{and}p=5.4\times 10^{-8},$$

$$\log S_{\mathrm{r}}^{\mathrm{de}-\mathrm{beamed}}=(0.79\pm 0.03)\log F_{\mathrm{o}}^{\mathrm{de}-\mathrm{beamed}}+(12.02\pm 0.42),r=0.88\mathrm{and}p=2.2\times 10^{-74},$$

$$\log F_{\mathrm{X}}^{\mathrm{de}-\mathrm{beamed}}=(0.48\pm 0.02)\log F_{\mathrm{o}}^{\mathrm{de}-\mathrm{beamed}}+(5.80\pm 0.28),r=0.86\mathrm{and}p=7.4\times 10^{-63},$$

$$\log F_{\mathrm{X}}^{\mathrm{de}-\mathrm{beamed}}=(0.53\pm 0.02)\log S_{\mathrm{r}}^{\mathrm{de}-\mathrm{beamed}}-(1.56\pm 0.03),r=0.85\mathrm{and}p=4.8\times 10^{-62},$$

$$\Gamma =\frac{{\beta }_{\mathrm{app}}^2+{\delta }^2+1}{2\delta },\tan \varphi =\frac{2{\beta }_{\mathrm{app}}}{{\beta }_{\mathrm{app}}^2+{\delta }^2-1}.$$

$$⟨{\delta }^{\mathrm{FDS}}⟩=17.23\pm 12.54\mathrm{and}⟨{\delta }^{\mathrm{non}-\mathrm{FDS}}⟩=9.48\pm 8.86,$$

$$⟨{\Gamma }^{\mathrm{FDS}}⟩=21.41\pm 21.59\mathrm{and}⟨{\Gamma }^{\mathrm{non}-\mathrm{FDS}}⟩=13.57\pm 12.75,$$

Full text

1. In terms of average values, FDSs have higher proper motions ($\mu$), apparent velocities ($\beta_{\rm app}$), Doppler factor ($\delta$), Lorentz factor ($\Gamma$), and smaller viewing angle ($\phi$). Nevertheless, there is no clear difference in co-moving viewing angles ($\phi_{\rm co}$). The results reveal that that FDSs show stronger beaming effect than non-FDSs.
2. In terms of correlations: (1) Both sources show positive, mutually correlated fluxes, which become closer in de-beamed fluxes; (2) With respect to apparent velocities and $\gamma$-ray luminosity, there is a tendency for the brighter sources to have higher velocities; (3) With regard to viewing angle and observed $\gamma$-ray luminosity, ${\rm log}\phi=-(0.23\pm 0.04){\rm log}L_{\rm\gamma}+(11.14\pm 1.93)$, while for the co-moving viewing angle and the intrinsic $\gamma$-ray luminosity, ${\rm log}\phi_{\rm co}=(0.09\pm 0.01){\rm log}L_{\rm\gamma}^{\rm in}-(1.73\pm 0.48)$. These correlations show that the luminous $\gamma$-ray sources have smaller viewing angles and a larger co-moving viewing angle, which indicate a stronger beaming effect in $\gamma$-ray emissions.

active galactic nuclei, jets, $\gamma$-rays, Correlations

PCAS: 98.54.Cm; 98.58.Fd; 95.85.Pw; 98.62.Ve

1 introduction

The nature of AGNs is still an open question in astrophysics. AGNs contain a broad wavelength band emission, from radio to very high energy (VHE) band. Blazars, as a very extreme subclass of AGNs, show rapid and high variability, high and variable polarization, variable and strong $\gamma$-ray emission and even superluminal motion (Fan et al. 2013a; Fan et al. 2013b). These extreme observational properties of blazars are due to the fact that they host a relativistic jet pointing to the observer (Blandford & Königl. et al. 1979). Blazars have two subclasses, namely BL Lacertae objects (BL Lacs) and flat spectrum radio quasars (FSRQs). BL Lacs show weak or no emission lines while FSRQs show strong emission line features. The classifications of blazars based on the spectral energy distributions (SEDs) can be found in Padovani & Giommi. (1995), Nieppola et al. (2006), Abdo et al. (2010a), Fan et al. (2016), Lin & Fan. (2018) and Zhang & Fan. (2019).

The $\gamma$-ray emissions of blazars have caught astronomers’ attention to investigate the mechanism of the high energetic $\gamma$-ray emissions. There have been two generations of $\gamma$-ray experiment, EGRET (the Energetic Gamma-Ray Experiment Telescope, on-board the $Compton\ Gamma-Ray\ Observatory$) and Fermi-LAT (Fermi Large Area $Gamma-Ray\ Space\ Telescope$), which provide us good opportunities to detect strong $\gamma$-ray sources. Based on the observations of EGRET, correlation analyses between the $\gamma$-ray emissions and those at lower energy bands have been performed to study the beaming effect ( Dondi & Ghisellini. 1995; Xie et al. 1997; Fan et al. 1999; Cheng et al. 2000, and reference therein). Fermi-LAT, a successor to ERGET, detected more than 1000 blazars (see Abdo et al. 2010b; Nolan et al. 2012; Acero et al. 2015; Ackermann. 2015). The strong $\gamma$-ray emissions in blazars suggest the existence of a relativistic beaming effect, which is discussed in many papers (see Arshakian et al. 2010; Fan et al. 2013a; Fan et al. 2013b; Fan et al. 2014; Fan et al. 2017; Fan & Ji. 2014; Giovannini et al. 2014; Giroletti et al. 2012; Kovalev et al. 2009; Massaro et al. 2013a; Massaro et al. 2013b; Pushkarev et al. 2010; Savolainen et al. 2010; Xiao et al. 2015; Pei et al. 2016; Yang et al. 2017; Yang et al. 2018a; Zhang & Fan. 2018). The $\gamma$-ray emissions are also used to estimate the beaming boosting factors (Doppler factors) for some $\gamma$-ray loud sources (Mattox et al. 1993; Dondi & Ghisellini. 1995; von Montigny et al. 1995; Cheng et al. 1999; Fan et al. 1999; Fan et al. 2013a; Fan et al. 2013b; Fan et al. 2014; Fan 2005). Yang et al. (2018b) studied the effective spectral index properties, then suggested that synchrotron self-Compton (SSC) model could explain the main process for highly energetic $\gamma$ rays in BL Lacs. Moreover, the DArk Matter Particle Explorer (DAMPE), was successfully launched into a sun-synchronous orbit at the altitude of 500 km on 2015 December 17th from the Jiuquan launch base. DAMPE offers a new opportunity for advancing our knowledge of cosmic rays, dark matter, and gamma-ray astronomy as well (Chang et al. 2017). This marks a new generation of astrophysics, which has bound particles physics and astronomy together tightly.

For blazars, the Doppler factor ($\delta=[\Gamma(1-\beta\rm{cos}\phi)]^{-1}$) is an important parameter, where $\Gamma=(1-\beta^{2})^{1/2}$ is a bulk Lorentz factor, $\beta$ is the jet speed in units of the speed of light, and $\phi$ is a viewing angle between the jet and the line-of-sight. The Doppler factor is a key quantity in jets since it determines how much flux densities are boosted and timescales compressed in the observer frame. The Doppler factor, although a crucial parameter in the blazar paradigm dictating all of the observed properties of blazars, is very difficult to estimate since there is no direct determining method for either $\beta$ or $\phi$. For this reason, many indirect methods have been proposed in order to estimate $\delta$, which usually involves different energetic (e.g., Ghisellini et al. 1993; Mattox et al. 1993; Fan et al. 2013a; Fan et al. 2014) and/or causality arguments (Lähteenimäki & Valtaoja. 1999; Hovatta et al. 2009; Jorstad et al. 2005; Jorstad et al. 2017; Liodakis et al. 2018) or fitting the spectral energy distribution (SED, Ghisellini et al. 2014; Zhang et al. 2012; Chen et al. 2018) of $\gamma$-ray emitting blazars. Lähteenimäki & Valtaoja. (1999) proposed to estimate the Doppler factor ($\delta_{\rm var}$) using radio flux density variations. They obtained the timescales for radio emissions, assumed the timescales to represent the emission size, and got a brightness temperature ($T_{\rm B}^{\rm ob}$). If the intrinsic brightness temperature is assumed to be $T_{\rm B}^{\rm in}=5\times 10^{10}\rm{K}$ and the difference between the two brightness temperatures is from the beaming effect, then a variation Doppler factor, $\delta_{\rm var}=(T_{\rm B}^{\rm ob}/T_{\rm B}^{\rm in})^{1/3}$ can be estimated. This method was used to estimate a large sample with longer coverage of radio observations (see Hovatta et al. 2009). Fan et al. (2009) and Savolainen et al. (2010) also adopted that method to estimate the Doppler factor in the radio band. Furthermore, the Doppler factor was also estimated for the $\gamma$-ray loud blazars, Fan et al. (2013a) and Fan et al. (2014) suggested a Doppler factor can be expressed as

[TABLE]

here $\Delta T$ is the time scale in units of hour, $\alpha$ is the X-ray spectral index, $F_{\rm{1KeV}}$ is the flux density at 1 KeV in units of $\rm{\mu Jy}$, $E_{\rm{\gamma}}$ is the energy in units of GeV, at which the $\gamma$-rays are detected, and $d_{\rm L}$ is luminosity distance in units of Mpc.

Superluminal motion is also an interesting observational property of blazars. Thanks to the very large baseline interferometry (VLBI) established by Europe, Canada, United States, Russia and so on, with high angular resolution at milliarcsecond, many AGNs show interesting observational results, some compact radio sources consist of more than one component, and some of these components seem to be separating at apparent velocities being greater than the speed of light. A parameter, $\beta_{\rm app}(=v/c)$, is introduced to value the apparent velocity. If $\beta_{\rm app}>1$, then it is called to be superluminal, and this kind of sources are called superluminal sources.

The first apparent superluminal motion was observed from 3C 279, a component moving away from the quasar core at nearly ten times the speed of light was detected. Vermeulen & Cohen. (1994) listed 66 extragalactic sources, from which they found multi-epoch VLBI internal proper motions, then investigated several modifications to a simple relativistic beam concept and its statistical effects on apparent velocity. They also checked the distribution of $\beta_{\rm app}$ for lobe-selected and core-selected quasars respectively and obtained the $\beta_{\rm app}$ for different object categories to be in general agreement with an AGN unification model. In 1996, Fan1996 compiled a sample of 48 superluminal motion sources to investigate the beaming effect, found that the core dominance is an indicator of the orientation of the emission, and proposed that the superluminal motion and beaming effect are probably the same things. Kellermann et al. (2003) presented a sample of 96 superluminal sources to study the nature of the relativistic beaming effect in blazars and their surrounding environment of the massive black holes. They found that most of the blazars show an outward flow away from the centre core while a few sources show the opposite direction of features, and there is no simple correlation between timescale of flux changes and apparent velocities. In 2008, Zhang & Fan. collected an up-to-date sample of 123 superluminal sources including 84 quasars, 27 BL Lac objects and 12 galaxies, calculated the apparent velocities for each source, and found that the radio emissions are strongly boosted by the beaming effect and the superluminal motion is the same thing as the beaming effect in AGNs.

For the details of kinematics in superluminal motion, Britzen et al. (2008) presented a detailed kinematic analysis of the complete flux-density limited Caltech-Jodrell Bank Flat-spectrum (named CJF 111http://www.mpifr-bonn.mpg.de/staff/sbritzen/cjf.html) sources. CJF survey computed 2D kinematic models based on the optimal model-fitting parameters of multi-epoch VLBA observations, then investigated possible correlations between the apparent proper motions and some other parameters in AGN jets. They found a strong correlation between the 5 GHz luminosity and apparent velocity. Based on the data of MOJAVE 222http://www.physics.purdue.edu/MOJAVE/ (Monitoring of Jets in Active galactic nuclei with VLBA Experiments) sample, Lister et al. (2009) discussed the jet kinematics of a complete flux-density-limited sample of 135 radio-loud AGNs resulting from a 13-years program, investigated the structure and evolution of parsec-scale jet phenomena, and found there is an overwhelming tendency to display outward motions, only eight inward moving components. Lister et al. (2013) studied 200 AGNs parsec-scale jet orientation variations and superluminal motion, found a general trend of increasing apparent speed with distance down the jet for both radio galaxies and BL Lac objects.

Since Fermi-LAT was launched in 2008, the 4-year catalogue includes 1591 AGNs. Although AGNs are the main detection result by Fermi-LAT, while there are many AGNs are not detected by Fermi. Why are some AGNs detected by Fermi-LAT and others are not? To answer this question, we compile a large superluminal sample (189 FDSs and 102 non-FDSs) and use them to make a comparison between the FDS and the non-FDS sources and do some statistical analyses. This work is arranged as follows: In section 1, we introduce our superluminal sample, in section 2, we will give results, and discussions and conclusions are presented in sections 3 and 4.

Through this paper, a $\Lambda$-CDM model with $\Omega_{\rm\Lambda}\simeq 0.7$, $\Omega_{\rm M}\simeq 0.3$ and $\Omega_{\rm K}\simeq 0.0$, and $H_{\rm 0}=73~{}{\rm{km\,s^{-1}}}{\rm{Mpc^{-1}}}$ is adopted.

2 Samples and Results

2.1 Samples

From the available literature, we compile 291 sources with superluminal motions, including 189 ( 142 FSRQs, 39 BL Lacs, 5 galaxies and 2 uncertain type blazar candidates (BCU) and 1 unknown type of AGN without a known redshift ) Fermi detected superluminal sources (FDS) and 102 ( 98 FSRQs, 1 BL Lac and 12 galaxies and 1 unknown type of AGN without a known redshift ) non-Fermi detected superluminal (non-FDS) sources, where Fermi detected sources mean these sources are detected by Fermi-LAT telescope and listed in the Fermi AGN catalogues.

There are 816 components for the 189 FDS sources in total, 30 of them have just one component. In the present sample, we also include the $\gamma$-ray emission source, 0007+106 (III ZW 2), which was classified as an $\gamma$-ray source by Liao et al. (2016). All the FDS sources are listed in Table 1.

For the 102 non-FDS sources ( 88 FSRQs, 1 BL Lac, 12 galaxies and 1 unknown type of AGN) with 400 components totally, 17 of them have just one component, they are in Table 2,

2.2 Results

2.2.1 Proper Motion and Apparent Velocity Distribution

For a proper motion ($\mu$), an apparent velocity ($\beta_{\rm app}$) can be computed by,

[TABLE]

Hence, we calculate apparent velocities from its given proper motions if its apparent velocities are not given by MOJAVE (Lister et al. 2013; Lister et al. 2016) or other reference literature for the sources in Tables 1 and 2. Then we compare their maximum proper motion ($\mu^{\rm max}$) and maximum apparent velocity ($\beta^{\rm max}_{\rm app}$), averaged proper motion ($\mu^{\rm mean}$) and averaged apparent velocity ($\beta^{\rm mean}_{\rm app}$) between FDS and non-FDS sources. The corresponding uncertainty of averaged value is expressed by an error-transmission format:

[TABLE]

The distributions of the maximum and averaged proper motion and the apparent velocity for FDS and non-FDS sources are shown in Figures 1-2, where the red stepped line is for FDS, and the blue stepped line for non-FDS sources.

It is found that the maximum proper motion is distributed from 0.018 to 2.510 with a mean value of $\langle\mu^{\rm max}_{\rm FDS}\rangle=0.361\pm 0.037\ {\rm mas}\cdot{\rm yr^{-1}}$ for the FDS sources, and from 0.021 to 2.941 with $\langle\mu^{\rm max}_{\rm non-FDS}\rangle=0.224\pm 0.027\ {\rm mas}\cdot{\rm yr^{-1}}$ for the non-FDS sources. When a Kolmogorov-Smirnov (K-S) test is adopted to the two distributions, the probability for the two distributions to come from the same distribution is $p=6.2\times 10^{-5}$, see Figure 1.

The mean proper motion is distributed from 0.011 to 1.853 with $\langle\mu^{\rm mean}_{\rm FDS}\rangle=0.233\pm 0.021\ {\rm mas}\cdot{\rm yr^{-1}}$ for the FDS sources and from 0.015 to 2.193 with $\langle\mu^{\rm mean}_{\rm non-FDS}\rangle=0.158\pm 0.015\ {\rm mas}\cdot{\rm yr^{-1}}$ for the non-FDS sources, and $p=1.6\times 10^{-4}$, see Figure 1.

From the calculations, it is found that the maximum apparent velocity $\beta^{\rm max}_{\rm app}$ is distributed from 1.04 to 39.70 with $\langle\beta_{\rm FDS}^{\rm max}\rangle=12.36\pm 1.64$ for the FDS sources and from 1.08 to 58.04 with $\langle\beta_{\rm non-FDS}^{\rm max}\rangle=8.75\pm 1.32$ for non-FDS sources, and $p=3.3\times 10^{-7}$, see Figure 2.

For the mean apparent velocity, $\beta^{\rm mean}_{\rm app}$ is distributed from 0.53 to 34.80 with $\langle\beta_{\rm FDS}^{\rm mean}\rangle=8.17\pm 0.94$ for the FDS sources and from 0.61 to 29.33 with $\langle\beta_{\rm non-FDS}^{\rm mean}\rangle=5.99\pm 0.78$ for non-FDSs, and $p=1.4\times 10^{-4}$, see Figure 2.

2.2.2 Correlations between Proper Motion and Redshift

From the data listed in Tables 1 and 2, when a linear regression fitting is adopted to the proper motion and redshift, we have

[TABLE]

with a correlation coefficient $r=-0.26$ and a chance probability of $p=4.0\times 10^{-4}$ for the FDSs, and

[TABLE]

with $r=-0.13$ and $p=20\%$ for the non-FDSs, see Figure 3.

2.2.3 Correlations between Apparent Velocity and Redshift

For the apparent velocity ($\beta_{\rm app}$), we have following results for the maximum and average values of apparent velocity ($\beta_{\rm app}$),

[TABLE]

[TABLE]

for the 186 FDSs (3 excluded sources without redshift from NED ), and

[TABLE]

[TABLE]

for the 101 non-FDS as shown in Figure 4.

2.2.4 Correlation between Apparent Velocity and $\gamma$-Ray Luminosity

For the $\gamma$-ray sources, the integral flux ($f$) in units of $\rm GeV\cdot cm^{-2}\cdot s^{-1}$, can be expressed in the form (Fan et al. 2013b)

[TABLE]

[TABLE]

here ${N_{(E_{\rm L}\sim E_{\rm U})}}$ is the integral photons in the energy range of $E_{\rm L}$ and $E_{\rm U}$. In this work, $E_{\rm L}$ and $E_{\rm U}$ are corresponding to 1 GeV and 100 GeV respectively. Then, we calculate the $\gamma$-ray luminosity ($L_{\gamma}$) in units of $\rm erg\cdot s^{-1}$ by

[TABLE]

here, $L_{\rm\gamma}$ is the $\gamma$-ray luminosity, $d_{\rm L}=\frac{c(1+z)}{H_{\rm 0}}\int^{1+z}_{1}\frac{1}{\sqrt{\Omega_{\rm M}x^{3}+1-\Omega_{\rm M}}}dx$ is a luminosity distance, $(1+z)^{(\alpha_{\rm{ph}}-2)}$ stands for a K-correction, $\alpha_{\rm{ph}}$ for $\gamma$-ray photon spectral index.

Figure 5 shows the maximum and average apparent velocity against the $\gamma$-ray luminosity. The dash curved upper envelope is described by Cohen et al. (2007), the upper envelope of this distribution traces out a single source of a given bulk Lorentz factor and intrinsic luminosity in the ($L$, $\beta_{\rm app}$) plane as the viewing angle $\phi$ changes. Such an aspect curve is plotted in Figure 5 for a jet with a bulk Lorentz factor of 42 and an intrinsic luminosity of log$L_{\rm in}$= 42, assuming Doppler boosting by a factor of $\delta^{3}$, by these formulas: $\delta=\frac{1}{\Gamma(1-\beta{\rm cos}\phi)},\beta_{\rm app}=\frac{\beta{\rm sin}\phi}{1-\beta{\rm cos}\phi},L=L_{\rm in}\delta^{3}.$

2.2.5 Flux Density-Flux Density Correlations

The multi-wavelength (radio, optical and X-ray) data are from the BZCAT, the optical magnitude is made galactic extinction correction and then transferred into optical flux density. The optical, radio and X-ray flux densities are also K-corrected by $(1+z)^{\alpha-1}$, where $\alpha$ ($F_{\nu}\propto\nu^{-\alpha}$) is the spectral index in the given band. For the spectral indexes, we adopt $\alpha_{\rm r}=0$ for radio band (Donato et al. 2001, Abdo et al. 2010a), while for optical band, $\alpha_{\rm o}=0.5$ for BLs and $\alpha_{\rm o}=1$ for the rest of the sources as did by Donato et al. (2001), $\alpha_{\rm X}=0.78$ for FSRQs, $\alpha_{\rm X}=1.30$ for BLs and $\alpha_{\rm X}=1.05$ for BCUs from Fan et al. (2016). For any two bands, we have

[TABLE]

[TABLE]

[TABLE]

for FDSs, and

[TABLE]

[TABLE]

[TABLE]

for non-FDSs. These corresponding results are shown in Figure 6.

For the subclasses of BL Lacs and FSRQs, their correlations are shown in Table 3 for FDSs and non-FDSs.

3 Discussions

As a subclass of AGNs, blazar has many extreme observation properties, which may be attributed to a relativistic beaming effect. We compile proper motions, $\mu$ for 1216 components for 291 sources, including 189 FDS and 102 non-FDS sources. Then we collect and calculate the corresponding apparent velocity ($\beta_{\rm app}$), get their multi-wavelength data, and Doppler factors from available references (BZACT, MOJAVA, Fermi-3rd catalogue, and so on), make comparisons between FDSs and non-FDSs, and then investigate some statistical correlations.

3.1 Averaged Values for Superluminal Motions

The averaged maximum values of proper motion for FDSs and non-FDSs are $\langle\mu^{\rm max}_{\rm FDS}\rangle=0.361\pm 0.037$ and $\langle\mu^{\rm max}_{\rm non-FDS}\rangle=0.224\pm 0.027$; while the averaged mean values of proper motion are $\langle\mu^{\rm mean}_{\rm FDS}\rangle=0.233\pm 0.021$ and $\langle\mu^{\rm mean}_{\rm non-FDS}\rangle=0.158\pm 0.015$ respectively. The averaged maximum values of apparent velocity for FDS and non-FDS sources are $\langle\beta^{\rm max}_{\rm FDS}\rangle=12.36\pm 1.64$ and $\langle\beta^{\rm max}_{\rm non-FDS}\rangle=8.75\pm 1.32$; the averaged mean values are $\langle\beta^{\rm mean}_{\rm FDS}\rangle=8.17\pm 0.94$ and $\langle\beta^{\rm mean}_{\rm non-FDS}\rangle=5.99\pm 0.78$.

Based on MOJAVE 1.5 Jy flux density-limited samples, Lister et al. (2016) get a less than 0.02 % probability that the LAT and non-LAT sub-samples come from the same parent distribution according to K-S tests. When a K-S test is adapted to these distributions of FDSs and non-FDSs, we find that probability for the distributions of FDSs and non-FDSs to be from the same distribution is less than $1.6\times 10^{-4}$ as shown in Figure 1-2, suggesting FDSs and non-FDSs should be from two different distributions. Our result confirms the result by Lister et al. (2016). We can say that FDSs have a larger proper motion and apparent velocity than do non-FDSs.

These results are consistent with other results. Jorstad et al. (2001) indicated that the sources with $\gamma$-ray emission show greater apparent velocities ($\beta_{app}$) than these sources without $\gamma$-ray emissions. Lister et al. (2009), Lister et al. (2016) and Piner et al. (2012) also confirmed this result, which means that the $\gamma$-ray sources are highly beamed. Our result based on the largest superluminal sample also confirms their results.

3.2 Correlations

Vermeulen & Cohen. (1994) collected 66 sources with proper motions, they showed that the proper motion decreases with increasing redshift (see also, Cohen et al. 2005). In our previous work (Zhang & Fan. 2008), we collected a sample of 123 superluminal sources, investigated the correlation between proper motion and redshift, and got ${\rm log}\mu\sim{-0.28}{\rm log}z$. In this paper, we obtained ${\rm log}\mu^{\rm max}=-(0.28\pm 0.07){\rm log}z-(0.95\pm 0.02)$ with $r=0.22$ and a chance probability of $p=1.2\times 10^{-4}$ for the whole sample. The result indicates clearly that the proper motion decreases with the increasing redshift, which is consistent with the results from others’ (Vermeulen & Cohen. 1994, Cohen et al. 2005 and Zhang & Fan. 2008). When we consider FDS and non-FDS separately, there is an anti-correlation with a slope of $-0.35$ for the FDSs, and an anti-correlation tendency with a slope of $-0.14$ for the non-FDSs.

When we investigate linear correlations between apparent velocities (log$\beta_{\rm app}$) and redshift (log$z$), slopes are 0.36 and 0.59 are obtained from the log$\beta_{\rm app}$-log$z$ fitting for FDS and non-FDS sources respectively, which means the apparent velocity increases with redshift. Obviously, for non-FDS, the positive correlation is much better which with a chance probability is $p=1.6\times 10^{-7}$. Lister et al. (2009) plotted maximum apparent velocity against redshift for their sample and showed that the maximum superluminal velocity increases with redshift. In the MOJAVE survey, the minimum detectable luminosity rises sharply with redshift, creating a classical Malmquist bias and the high redshift sources have higher apparent luminosities, which they achieved primarily via Doppler boosting (Lister et al. 2009). Our result is consistent with theirs.

Kellermann et al. (2007) quoted their result of apparent velocity and luminosity and indicated that there are no low luminosity sources with fast motions. The high luminosity sources show a wider range of apparent velocity. In Figure 5, we also find such a tendency that the brighter $\gamma$-ray sources show a higher apparent velocity. It is due to a beaming effect because a source with a higher velocity suggests a corresponding higher Doppler factor, and a higher Doppler boosting results in a higher luminosity.

From Fig. 5, we can see a tendency for higher apparent velocity source to have higher $\gamma$-ray luminosity. However, we can also see that some luminous $\gamma$-ray source have also low apparent velocity. Actually, there is an envelope between apparent velocity and $\gamma$-ray luminosity in Figure 5, which is similar to that seen in the Caltech-Jodrell Bank Flat Spectrum (CJF) survey (Vermeulen. 1995), the 2 cm Survey (Kellermann et al. 2004), and the MOJAVE survey (Cohen et al. 2007; Lister et al. 2009; Piner et al. 2012). This upper envelope is not due to selection effects, although its precise physical origin is unclear. Lister et al. (2009) speculated that such an envelope may arise because of an intrinsic relation between jet speed and luminosity in the parent population.

3.3 Flux-Flux Correlations

The mutual correlations between fluxes were investigated in literature. Fan et al. (1994) compiled 52 X-ray selected BL Lacs to study the mutual correlations among radio, X-ray and optical data and found closely mutual correlations. Dondi & Ghisellini. (1995) studied correlations between $\bar{L}_{\rm\gamma}$ versus $\bar{L}_{\rm r}$, $\bar{L}_{\rm o}$ and $\bar{L}_{\rm X}$, for a sample of quasars detected by EGRET, obtained positive correlations, and found that $\bar{L}_{\rm\gamma}$ correlates closer with $\bar{L}_{\rm r}$ than with $\bar{L}_{\rm o}$ or $\bar{L}_{\rm X}$. In the present work, we investigate mutual correlations for radio, optical and X-ray fluxes for both FDS and non-FDS sources. For our flux-flux correlation analysis, we can see positive correlations and that there is no significant difference in slopes and intercepts between FDSs and non-FDSs. In 2010, Abdo et al. used quasi-simultaneous data to calculate the SEDs for a sample of 48 LAT Bright AGN sample sources (LBAS). From their multwavelength data, we get following corresponding results,

[TABLE]

[TABLE]

[TABLE]

We can see that the results based on the quasi-simultaneous data are similar to our results.

The emissions from AGNs are mainly from the jet, however there are contaminations from the host galaxy (especially for BL Lac objects) as well as the big blue bump (especially for FSRQs) in the optical band, together with the contribution from the accretion system in the X-ray domain. Since the sample considered here is all superluminal, their jet emission should be strongly boosted, which make the contaminations in the optical and X-ray bands be relatively small.

Ghisellini et al. (1989) proposed that the bulk velocity of the plasma increases with distance from the core and synchrotron X-rays are weakly beamed, while optical and radio emissions are more strongly beamed. Fan et al. (1993) proposed an empirical frequency dependent Doppler factor: $\delta_{\rm\nu}=\delta_{\rm o}^{1+1/8~{}{\rm log}({\nu}_{\rm o}/{\nu})}$, where $\delta_{\rm o}$ is the optical Doppler factor, then $\delta_{\rm X}\sim\delta_{\rm o}^{0.5}$, $\delta_{\rm r}\sim\delta_{\rm o}^{1.5}$, $\delta_{\rm X}$ and $\delta_{\rm r}$ are the X-ray and radio Doppler factors (Fan et al. 1993). In a beaming model, the observed emission, $f^{\rm ob}$, is strongly boosted, namely, $f^{\rm ob}=\delta^{p}f^{\rm in}$, here $f^{\rm in}$ is the intrinsic emission in the source frame, $\delta$ is the Doppler factor, $p=3+\alpha$ is for a moving compact source or $p=2+\alpha$ for a continuous jet (Lind & Blandford. 1985). Here $p=2+\alpha$ is used as we did before (Xiao et al. 2015). In the work, Doppler factors are available for 224 sources, which makes it possible for us to investigate the mutual correlations for the intrinsic (de-beamed) radio, optical and X-ray flux emissions. For the 224 sources, we have

[TABLE]

[TABLE]

[TABLE]

for the observed data; and

[TABLE]

[TABLE]

[TABLE]

for the intrinsic data. It is clear that the correlations between any two bands become much closer when the beaming effect is removed. The result indicates that the beaming effect affects the observed broad band correlations. The comparison results are shown in Figure 7.

3.4 Basic parameters for Jets

3.4.1 Doppler Factor, Lorentz Factor and Viewing Angle

Doppler factors are important but not easy to estimate, although several methods were proposed. In the present work, we collect Doppler factor for 229 sources (151 FDS and 78 non-FDS) and list them in Column 4 in Tables 1 and 2.

In a beaming model, the Lorentz factor ($\Gamma$) and viewing angle ($\phi$) can be obtained from $\delta$ and $\beta_{\rm app}$:

[TABLE]

From the Doppler factors in Tables 1 and 2, we have,

[TABLE]

a K-S test result shows that the probability for the two distributions to be from the same one is $7.5\times 10^{-7}$.

For the sources with available Doppler factors, we can calculate $\Gamma$ and $\phi$, and get their mean values:

[TABLE]

and

[TABLE]

with chance probabilities being $p=5.2\times 10^{-5}$ and $p=1.5\times 10^{-7}$ respectively, which show significant difference in Lorentz factor and viewing angle between FDS and non-FDS sources.

Savolainen et al. (2010) obtained that for the photons arriving to us at an angle $\phi$, the jet flow is at an angle $\phi_{co}$ in the co-moving frame:

[TABLE]

then, from the obtained $\Gamma$ and $\phi$, we can get $\phi_{co}$, and their mean values are

[TABLE]

with a K-S test result of $p=15.8\%$ suggesting no clear difference in co-moving viewing angle between FDSs and non-FDSs.

From K-S test results, we can see that there are significant differences in Doppler factor, viewing angle and Lorentz factor between FDSs and non-FDSs. FDSs show higher Doppler factors, higher Lorentz factor, and smaller viewing angle than do non-FDSs. The fact that FDS sources have larger Doppler factor also confirmed by Lister et al. (2015) who used the MOJAVE sample as well. However, the co-moving viewing angles show no clear difference between FDSs and non-FDSs. It means that FDS and non-FDS jets have similar cone in the comoving frame.

Above analysis results suggest that the difference between Fermi detected superluminal sources and non-Fermi detected superluminal sources comes from their difference beaming effect with FDSs being strongly beamed than non-FDSs. The superluminal source 0007+106 (III ZW2) was not listed in the 3FGL, but it was classified as a $\gamma$-ray source by Liao et al. (2016). So, we propose that the superluminal source is a $\gamma$-ray candidate and the $\gamma$-ray source should be a superluminal source. Our sample gives that $\langle\beta^{\rm max}_{\rm non-FDS}\rangle=8.75\pm 1.32$ for non-FDS sources, and $\langle\beta^{\rm max}_{\rm FDS}\rangle=12.36\pm 1.64$ for the FDS sources. If we take non-Fermi sources with $\beta^{\rm max}_{\rm non-FDS}>\langle\beta^{\rm max}_{\rm FDS}\rangle+5\sigma$ as the candidate of $\gamma$-ray emitter, then there are 6 $\gamma$-ray emitting candidates, and they are 0153+744, 0208-512, 0536+145, 0552+398, 2223+210, 2351+456.

3.4.2 $\gamma$-ray Luminosity and Viewing Angle

For $\gamma$-ray luminosity ($L_{\rm\gamma}$) and viewing angle ($\phi$), there is a significant anti-correlation,

[TABLE]

with $r=-0.38~{}{\rm and}~{}p=2.2\times 10^{-6}$. The best fitting result is shown in Figure 8 with a solid line. The results imply that the more luminous $\gamma$-ray sources have smaller viewing angles.

However, in a beaming model, the observed flux density, $f^{\rm ob}$ is correlated with the intrinsic flux density, $f^{\rm in}$, by $f^{\rm ob}=\delta^{p}f^{\rm in}$, where $p=3+\alpha$ for a discrete case and $p=2+\alpha$ for a continuous case. So, for the luminosity, we have $L^{\rm ob}=\delta^{4+\alpha}L^{\rm in}$ for a discrete case, or $L^{\rm ob}=\delta^{3+\alpha}L^{\rm in}$ for the continuous case. For sources with available $\delta$, we can get their intrinsic luminosity and co-moving viewing angle, which show

[TABLE]

with $r=0.69~{}{\rm and}~{}p=7.3\times 10^{-22}$, the result is shown in Figure 9 with a solid line.

Obviously, there is a positive correlation between co-moving viewing angle and intrinsic luminosity, which suggests that the luminous intrinsic $\gamma$-ray luminosity corresponds to a wider co-moving viewing angle. If the emission per solid angle in the comoving is similar for Fermi-LAT sources, then the larger co-moving angle corresponds to larger solid angle frame, then the emission is stronger.

From Figures 5-9, we can see that FDS and non-FDS sources are different. FDSs show higher proper motion ($\mu$), higher apparent velocity ($\beta_{\rm app}$), higher Doppler factor ($\delta$), higher Lorentz factor ($\Gamma$) and smaller viewing angle ($\phi$) than non-FDSs. We can say that FDSs have stronger beaming effect than do non-FDSs.

4 Conclusions

The 291 superluminal sources had 1216 components. We collected their multi-wavelength data and Doppler factors and calculated the apparent velocity for each component, the Lorentz factor and viewing angle (co-moving angle) for those with an available Doppler factor, calculate the $\gamma$-ray luminosity for the 3GFL sources. Subsequently, we investigated the relationships between FDS and non-FDS sources. Our main conclusions are summarized as follows:

1. FDS sources show higher proper motion, apparent velocity, Doppler factor, Lorentz factor and smaller viewing angles than non-FDS sources. For superluminal sources, FDSs are more beamed.

2. The intrinsic (de-beamed) fluxes show much closer mutual correlations among radio, optical and X-ray bands than the observed data.

3. A higher apparent velocity source has the tendency to exhibit higher $\gamma$-ray luminosity, and the superluminal sources may be the $\gamma$-ray emission candidates; moreover $\gamma$-ray sources with no known superluminal velocity can be superluminal candidates.

4. The $\gamma$-ray brighter source shows a smaller viewing angle, which suggest a strong Doppler effect. High energetic $\gamma$-ray emissions per solid angle are probably similar in the co-moving frame; thus the de-beamed $\gamma$-ray luminosity is positively correlated with the co-moving viewing angle.

This work is partially supported by the National Natural Science Foundation of China (NSFC 11733001, NSFC U1531245, NSFC 10633010, NSFC 11173009,NSFC 11403006), Natural Science Foundation of Guangdong Province (2017A030313011), supports for Astrophysics Key Subjects of Guangdong Province and Guangzhou City, and Science and Technology Program of Guangzhou (201707010401). We also thank the MOJAVE team and Purdue University for use the precious data of kinematic details. We thank the referees for the useful comments and constructive suggestions.

Appendix A Appendix: Full version of Tables

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