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Table 4

Results from the VLBA data.

RA Dec zabs rms Id S r θ a b/a φ ST fVLBA/ LS α
cf
(J2000) (J2000) (mJy beam-1) (mJy) (mas) (deg) (mas) (deg) (mJy) (pc)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13) (14) (15)
VLBA parameters at 20-cm
 01 08 26.8432 –00 37 24.060 1.3710 1.8 1 489 0  −  6.36 0.54 78 930 0.97/ 554 0.38
2 162 16.8 80 29.90 0.12 –78 0.53
3 58 33.1 88 21.35 0.29 –33
4 90 51.4 87 13.61 0.39 –84
5 106 65.3 79 21.71 0.64 –64
 01 54 54.3653 –00 07 23.231 1.1803 0.3 1 250 0  −  6.83 0.16 –38 264 0.95  < 57 –0.65
 02 14 52.2909 +14 05 27.455 1.4463 0.2 1 11 0  −  4.24 0.00 68 125 0.11/ 113 0.68
2 3 13.3 57 10.99 0.54 –23 0.09*
 02 40 08.1758 –23 09 15.727 1.3647 2.3 1 4080 0  −  4.75 0.85 39 6256 0.85/ 84 –0.25
2 1224 9.9 22 4.85 0.29 24 0.65
 02 59 28.5155 –00 19 59.983 1.3370 0.3 1 231 0  −  3.51 0.36 –10 235 0.98  < 30 –0.55
 07 42 37.3873 +39 44 35.629 1.1485 0.3 1 74 0  −  5.98 0.17 –27 114 0.76/ 63 0.35
2 13 7.6 155 6.65 0.83 0 0.65*
 07 48 09.4683 +30 06 30.533 1.4470 0.3 1 105 0  −  28.33 0.50 –85 231 0.65/ 464 0.49
2 20 30.1 0 14.31 0.00 –85 0.46*
3 24 28.8 135 71.92 0.23 –79
 08 00 36.0269 +50 10 44.290 1.4146 0.3 1 81 0  −  4.22 0.04 33 118 0.81/ 286 0.08
2 14 33.6 24 16.1 0.19 19 0.69*
 08 02 48.4323 +29 17 34.211 1.3648 0.3 1 7 0  −  3.94 0.42 –72 195 0.04*  < 33 0.88
 08 08 39.6666 +49 50 36.529 1.4071 2.1 1 482 0  −  2.03 0.51 –53 930 0.52  < 17 –0.25
 08 15 34.1624 +33 05 29.010 0.8515 0.2 1 25 0  −  3.96 0.16 26 343 0.07  < 30 0.59
 08 17 10.5482 +23 52 23.970 1.3060 0.3 1 105 0  −  3.81 0.12 –65 215 0.84/ 122 0.15
2 71 5.92 –44 4.73 0.00 66 0.49
3 5 14.5 –89 6.67 0.00 53
 08 45 06.2503 +42 57 18.393 1.1147 0.3 1 164 0  −  2.20 0.55 46 218 0.75  < 18 0.03
 08 50 42.2438 +51 59 11.654 1.3265 0.2 1 65 0  −  1.80 0.10 –89 63 1.03  < 15 0.02
 08 52 44.7391 +34 35 40.521 1.3095 0.3 1 47 0  −  2.39 0.67 64 69 0.74/ 60 –0.36
2 4 7.1 –124 8.69 0.00 –57 0.68
 09 30 35.0851 +46 44 08.579 0.6216 0.4 1 171 0  −  11.4 0.11 23 336 0.63/ 92 0.49
2 40 13.5 –154 13.6 0.39 15 0.51*
 09 53 27.9565 +32 25 51.525 1.2372 0.3 1 78 0  −  4.13 0.28 –1 132 0.71/ 161 0.14
2 16 19.3 0 11.0 0.34 –1 0.59
 10 07 18.0731 +22 51 26.955 0.5602 0.2 1 150 0  −  8.16 0.52 –64 350 0.55/ 49 0.54
2 42 7.6 –112 17.8 0.45 –7 0.43
 10 58 13.0427 +49 39 36.046 1.2120 0.2 1 5 0  −  15.3 0.00 64 244 0.33/ 840 0.70
2 27 20.9 92 7.98 0.00 90 0.11*
3 23 35.8 97 5.26 0.00 –81
4 6 56.9 –99 22.7 0.00 64
5 20 66.7 –107 12.7 0.98 –62
 11 00 21.0333 +16 29 14.661 0.8540 0.4 1 201 0  −  3.20 0.41 9 265 0.76  < 25 0.22
11 26 57.6554 +45 16 06.286 1.3022 1.4 1 340 0  −  3.42 0.66 21 424 0.80  < 24 –0.21
 11 48 56.5677 +52 54 25.337 0.8306 0.2 1 53 0  −  1.97 0.65 –69 100 0.78/ 56 0.38
2 25 7.36 116 3.70 0.00 –75 0.53
 11 57 34.8393 +16 38 59.769 0.7624 0.6 1 845 0  −  1.65 0.00 –80 747 1.00  < 12 –1.13
 12 08 54.2565 +54 41 58.163 1.2110 1.1 1 228 0  −  2.24 0.34 –51 265 0.86  < 11 0.04
 12 13 32.1710 +13 07 20.892 0.7718 1.4 1 145? 0  −  4.96 0.44 12 1356 0.11  < 37 0.45
 12 32 56.6101 +57 22 14.208 1.3429 0.2 1 4 0  −  7.33 0.39 –45 115 0.17/ 164 0.79
2 15 19.3 –150 37.57 0.19 26 0.13*
 12 34 31.7244 +64 55 56.530 1.3739/ 0.3 1 22 0  −  3.95 0.00 56 93 0.43/ 64 0.49
1.3829 2 18 7.5 0 10.14 0.74 23 0.24*
 13 00 36.4392 +08 28 02.887 0.8665 0.3 1 50 0  −  4.86 0.21 3 106 0.68/ 173 0.34
2 18 12.2 –178 6.32 0.26 24 0.47
3 4 22.4 –170 7.60 0.00 –20
 13 29 01.4156 +10 53 04.807 0.6715/ 0.2 1 34 0  −  3.60 0.00 –79 121 0.33/ 72,86 0.41
1.1645 2 6 10.3 81 9.80 0.69 9 0.28*
 13 33 35.7804 +16 49 04.109 0.7448 0.4 1 217 0  −  2.49 0.00 25 421 0.76/ 151 0.29
2 101 20.6 21 12.8 0.14 22 0.52
 14 08 56.4815 –07 52 26.635 1.2753 0.4 1 233 0  −  2.24 0.53 43 612 0.79/ 182 0.24
2 150 7.14 –106 4.35 0.00 48 0.38
3 77 13.5 –118 11.6 0.00 –85
4 25 8.35 47 11.0 0.37 –18
 14 10 30.9982 +61 41 36.908 0.7596 0.2 1 104 0  −  1.78 0.92 40 118 0.88  < 13 –0.41
 14 30 09.7389 +10 43 26.865 1.2431 0.8 1 301 0  −  1.69 0.46 65 311 0.97  < 14 –0.91
 15 01 24.6285 +56 19 49.678 1.2788 0.3 1 36 0  −  1.69 0.70 86 182 0.31/ 29 0.25
2 21 3.4 –117 9.97 0.00 64 0.20*
 15 08 23.7169 +33 47 00.762 1.1650 0.3 1 123 0  −  12.48 0.15 –45 132 0.99/ 126 0.61
2 7 15.2 –37 10.44 0.00 0 0.93
 16 23 46.2300 +07 18 54.891 1.3350 0.3 1 30 0  −  4.64 0.89 24 72  < 0.42* 39 0.82
 16 36 38.1833 +21 12 55.558 0.8000 0.4 1 147 0  −  2.06 0.69 –83 392 0.52/ 193 0.34
2 38 8.75 108 3.64 0.50 –58 0.38
3 7 9.11 –121 8.63 0.00 –47
4 13 19.3 113 14.4 0.47 10
 20 31 54.9948 +12 19 41.363 1.1157 0.2 1 447 0  −  2.58 0.40 4 985 0.48/ 76 –0.60
2 23 9.26 –173 10.4 0.10 –28 0.45
 23 40 23.6695 –00 53 27.009 1.3603 0.3 1 106 0  −  1.71 0.46 16 117 0.91  < 15 –1.20
 23 58 10.8819 –10 20 08.624 1.1726 0.4 1 571 0  −  3.71 0.29 –12 770 0.74  < 31 –0.70
VLBA parameters at 13-cm based on images from VCS
 04 57 03.1792 –23 24 52.020 0.8922 4.4  −   −   −   −   −   −   −  1760 0.63  < 195 –0.16
 11 45 21.3153 +04 55 26.690 1.3433 0.5  −   −   −   −   −   −   −  554 0.60/ 254 +0.55
0.32
 21 29 12.1759 –15 38 41.041 0.6628 1.0  −   −   −   −   −   −   −  990 0.89  < 140 –1.04

Notes. Columns 1 and 2: right ascension and declination of the “component-1” (see Col. 5) fitted to the quasar, respectively; Col. 3: absorption redshift; Col. 4: rms in the map in mJy beam-1; Col. 5: component id; Col. 6: flux of the component in mJy; Cols. 7 and 8: radius and position angle of the component with respect to “component-1”, respectively; Col. 9: major axis in mas of the Gaussian component fitted to characterise the milliarcsecond scale structure; Cols. 10 and 11: axial ratio and position angle of the Gaussian component, respectively; Col. 12: flux density in mJy from FIRST/NVSS (ST); Col. 13: ratio of total flux density detected in VLBA map and ST (called fVLBA). In case of quasars with the multiple Gaussian components the cf i.e. the ratio of the flux density of the strongest component detected in the VLBA map and the ST is also given; Col. 14: largest linear size (LS) i.e. separation between the farthest components of the quasar in pc at absorber redshift. For the quasars represented by a single Gaussian component we take major axis of the deconvolved component as the upper limit on quasar size; Col. 15: spectral index, S ∝ ν − α, between the 20-cm and 50-cm/90-cm using flux densities from the arcsecond scale maps.

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