Exploring the bulk of the BL Lacertae object population - I. Parsec-scale radio structures

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Table 2

Images parameters of 8 GHz and 15 GHz observations.


		8 GHz			15 GHz


Name	HPBW	rms	S _peak	HPBW	rms	S _peak
IAU	mas × mas, deg	mJy beam^-1	mJy beam^-1	mas × mas, deg	mJy beam^-1	mJy beam^-1


J0751+1730^1,2	–	–	–	–	–	–
J0751+2913³	–	–	–	1.2 × 0.8, –23.2	0.6	–
J0753+2921	1.8 × 1.1, 28.3	0.3	–	0.7 × 0.5, 4.5	0.4	–
J0754+3910	1.7 × 0.9, –33.0	0.2	23.3	1.3 × 0.5, –30.8	0.8	13.7
J0809+3455	2.0 × 1.0, –32.2	0.2	49.9	1.2 × 0.8, –29.9	0.4	45.8
J0809+5218	1.8 × 1.6, –12.8	0.2	61.5	2.1 × 1.6, 39.7	0.2	61.8
J0810+4911	1.0 × 0.8, –0.9	0.2	–	0.5 × 0.5, –28.9	0.6	–
J0847+1133¹	–	–	–	2.1 × 1.9, –31.1	1.1	–
J0850+3455	2.3 × 1.3, –29.8	0.1	22.1	1.7 × 1.7, –86.2	0.2	21.1
J0903+4055	1.2 × 1.0, –30.1	0.2	8.4	2.0 × 1.5, 20.1	0.3	5.9
J0916+5238	2.1 × 1.6, 13.7	0.3	25.3	3.2 × 2.2, 7.4	0.6	16.8
J0930+4950	2.2 × 1.6, –24.5	0.3	5.0	1.6 × 1.6, 37.1	0.2	4.4
J1012+3932	1.2 × 0.9, 38.5	0.3	–	1.0 × 0.5, –46.9	0.5	–
J1022+5124	1.2 × 0.9, –46.5	0.2	–	1.0 × 0.4, –59.7	0.6	–
J1053+4929	1.6 × 1.5, –42.2	0.2	25.7	2.4 × 1.8, –78.5	0.5	23.2
J1058+5628	1.9 × 1.7, –78.7	0.1	129.3	0.8 × 0.7, 84.8	0.3	95.0
J1120+4212	2.1 × 1.3, –4.5	0.2	16.2	1.9 × 1.4, 28.6	0.2	11.6
J1136+6737	2.2 × 1.1, 43.4	0.3	22.8	1.4 × 0.9, –58.6	0.2	16.0
J1145-0340	1.8 × 0.9, 3.7	0.4	–	1.0 × 0.4, –0.2	0.3	–
J1156+4238	1.6 × 1.5, –26.0	0.2	2.2	1.0 × 0.9, 6.5	0.1	1.3
J1201-0007^1,2	–		–	–	–	–
J1201-0011	3.4 × 1.5, –22.4	0.2	–	4.5 × 0.8, –27.4	1.0	–
J1215+0732	1.9 × 1.4, –5.7	0.3	27.3	1.3 × 0.8, –4.4	0.3	13.7
J1217+3007	2.8 × 2.8, –37.6	0.2	232.9	1.1 × 0.9, –7.3	0.3	187.0
J1221+0821²	3.3 × 1.6, –12.0	0.1	15.4	–	–	–
J1221+2813	1.8 × 1.4, –5.73	0.2	200.6	1.0 × 0.7, –11.1	1.0	168.3
J1221+3010	1.4 × 0.9, –3.8	0.2	27.9	3.0 × 0.6, –30.6	0.2	28.2
J1231+6414^1,2	1.8 × 1.5, 45.8	0.1	28.8	–	–	–
J1253+0326	3.4 × 1.2, –19.5	0.2	34.3	1.7 × 0.5 –20.3	0.4	23.9
J1257+2412	1.4 × 0.9, 0.0	0.3	–	0.8 × 0.5, –4.4	0.3	–
J1341+3959	3.4 × 2.0, –62.5	0.2	5.6	1.0 × 0.5, –22.4	0.3	4.8
J1419+5423	2.4 × 2.3, 20.9	0.3	802.4	1.1 × 0.8, –8.6	1.2	556.6
J1427+3908	1.3 × 1.0, –13.4	0.2	–	0.6 × 0.5, 5.43	0.3	–
J1427+5409¹	–	–	–	0.5 × 0.4, –7.8	0.4	5.1
J1428+4240	2.1 × 1.0, –30.3	0.2	21.4	1.5 × 0.4, –19.9	1.8	13.3
J1436+5639	2.6 × 1.5, –50.4	0.1	4.6	0.6 × 0.5, 10.8	0.2	3.6
J1442+1200	2.8 × 1.0, –22.8	0.2	25.4	3.3 × 0.8, –20.69	0.8	19.5
J1510+3335	1.2 × 0.9, –5.7	0.3	–	0.6 × 0.5, –6.4	0.3	–
J1516+2918	2.4 × 1.0, –24.6	0.2	27.7	1.8 × 0.7, –26.4	0.4	25.8
J1534+3715	1.2 × 1.0, –8.0	0.3	–	0.6 × 0.5, –1.1	0.3	–
J1604+3345	1.5 × 1.0, –33.2	0.2	–	0.9 × 0.5, –30.9	0.4	–
J1647+2909	2.1 × 1.2, –26.1	0.3	50.1	1.2 × 0.9, –22.1	0.8	46.5

Notes. Column 1: source names, where and

^(1,2)

is for undetected sources that were not observed in phase referencing mode at 8 and 15 GHz, respectively;

⁽³⁾

indicates the source that is not observed during all observational blocks in the project. We also list the half-power beam width (HPBW, Cols. 2 and 5), the rms (Cols. 3 and 5), and the flux density peaks (Cols. 4 and 7) for images at 8 and 15 GHz, respectively.

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