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This article has an erratum: [https://doi.org/10.1051/0004-6361/201833399e]


Table 2.

1.6 GHz VLBI and 1.5 GHz VLA properties of the VLBI detected sources.

Source ID z z typec/ref RA (J2000) Dec (J2000) VLBI P [μJy beam−1] VLBI I [μJy] S/N Beam [mas × mas (deg)] VLA P [μJy beam−1] VLA I [μJy]
(1) (2–4) (5,6) (7) (8) (9,10) (11,12) (13) (14–16) (17,18) (19,20)
J123555+620902a 1.8750 Sd 12:35:55.1267 +62:09:01.738 100.0+18.2 100.0±18.2 7.4 16.0×15.2(87.1) 165±17 192+ 19
J123607+620951 0.6380 Sd 12:36:06.6120 +62:09:51.159 118.0 + 22.8 118.0 + 21.2 6.1 5.3×4.6(3.0) 169±17 205 + 21
J123608+621036a 0.6790 Sd 12:36:08.1193 +62:10:35.906 122.0+16.8 140.0+18.2 11.1 16.0×15.4(86.8) 202± 20 236± 24
J123618+621541 1.9930 Se 12:36:17.5546 +62:15:40.765 177.0 + 25.0 192.0±26.0 10.1 5.4×4.6(10.6) 226± 23 275± 28
J123620+620844 1.0164 Sd 12:36:20.2620 +62:08:44.268 185.0 + 25.8 185.0±24.0 10.3 5.3×4.6(3.3) 141±14 156±16
J123621+621708a 1.9920 Sf 12:36:21.2684 +62:17:08.459 96.5± 14.5 135.0±17.3 8.9 15.6×15.3 (-8.2) 138±14 190±19
J123623+620654a Pg 12:36:22.5086 +62:06:53.844 114.0+19.0 144.0±21.4 8.2 16.1×15.3(86.3) 222± 22 249± 25
J123624+621643 1.9180 Se 12:36:23.5437 +62:16:42.746 222.0 + 28.2 383.0±42.0 12.8 5.4×4.5(10.6) 384±39 411±41
J123641+621833 1.1456 Sd 12:36:40.5661 +62:18:33.081 141.0 + 26.3 141.0±25.7 7.5 5.3×4.5(9.4) 293± 30 302±30
J123642+621331 2.0180 Sh 12:36:42.0899 +62:13:31.428 97.4+18.0 233.0±27.9 6.5 5.4×4.5(12.6) 432± 44 477± 48
J123644+621133 1.0128 Sd 12:36:44.3860 +62:11:33.170 410.0 + 44.8 411.0±44.7 25.9 5.3×4.5(11.4) 737± 74 1710± 171
J123646+621405 0.9610 Sd 12:36:46.3307 +62:14:04.692 191.0 + 24.9 192.0±24.8 12.3 5.4×4.5(12.7) 260± 26 280± 28
J123650+620738a 1.6095 Sd 12:36:49.6399 +62:07:37.844 77.3± 17.3 98.7±19.9 6.5 15.4×14.8(80.9) 267± 27 301±30
J123653+621444a 0.3208 Sd 12:36:52.8827 +62:14:44.069 109.0±15.1 117.0±15.6 11.0 14.8×14.7(9.6) 188±19 215±22
J123659+621833 Pg 12:36:59.3327 +62:18:32.566 2530.0±328.9 4430.0±572.7 88.2 5.3×4.5(8.5) 4250± 427 4640± 464
J123700+620910 Pg 12:37:00.2460 +62:09:09.779 153.0±23.4 163.0±24.1 9.4 5.3×4.5(8.0) 272± 27 319±32
J123709+620838 0.9070 Sl 12:37:09.4300 +62:08:37.587 125.0±21.4 127.0±21.5 7.3 5.3×4.5(6.4) 155±16 163±16
J123714+621826 3.44m Pi 12:37:13.8694 +62:18:26.301 501.0±56.8 629.0±69.4 25.6 5.3×4.6(6.9) 575±58 637± 64
J123715+620823 0.9335 Sj 12:37:14.9391 +62:08:23.223 2680.0± 272.9 2810.0±284.0 103.0 5.3×4.6(5.4) 1940±195 2090± 209
J123716+621512 0.5605 Sd 12:37:16.3730 +62:15:12.343 125.0±20.3 125.0±19.7 7.9 5.4×4.6(9.9) 165±17 178±18
J123717+621733 1.1460 Sd 12:37:16.6800 +62:17:33.310 150.0±23.8 269.0±32.7 8.2 5.4×4.6(7.5) 308±31 356±36
J123720+620741a Pk 12:37:20.0139 +62:07:41.410 94.8±14.6 112.0±15.8 8.8 15.9×15.4(67.2) 122±13 132±13
J123721+621130 Pg 12:37:21.2517 +62:11:29.961 328.0±38.3 364.0±41.6 20.2 5.3×4.5(8.8) 338±34 385±39
J123726+621129a 0.9430 Sj 12:37:25.9475 +62:11:28.699 124.0±16.7 142.0±18.2 12.2 15.4×15.1(52.6) 1190±120 5210±521
J123649+620439b 0.1130 Sd 12:36:48.9965 +62:04:38.850 >92.6 >102.0 10.5 12.5×11.6(1.2) 608±61 834± 83
J123701+622109b 0.8001 Sd 12:37:01.1023 +62:21:09.623 >111.0 >154.0 11.5 12.4×11.0(3.2) 285± 29 390±39
J123739+620505b Pk 12:37:39.3204 +62:05:05.489 >154.0 >194.0 11.6 12.1×10.9(5.6) 223± 23 258± 26
J123751+621919b Pk 12:37:51.2327 +62:19:19.012 >111.0 >181.0 8.8 11.9×10.5(0.5) 136±14 155±16
J123523+622248b Pk 12:35:22.6144 +62:22:48.028 >92.5 >144.0 7.3 12.1×10.6(7.0) 1260±126 1690±169
J123510+622202b Pk 12:35:10.2698 +62:22:02.067 >88.9 >91.4 7.9 12.1×10.6(7.0) 931±94 1280±128
J123656+615659b pk 12:36:55.8230 +61:56:58.917 >518.0 >528.0 12.7 9.6×9.0(39.0) 3590±361 26700± 2670

Notes. z: redshift, RA: Right Ascension (J2000), Dec: Declination (J2000), VLBI P: VLBI peak brightness (μJy beam−1), VLBI I: VLBI integrated flux density (μJy), N: noise (μJy beam−1), S/N: signal-to-noise, Beam: restoring beam in milliarcseconds and beam angle in degrees (major axis×minor axis (beam angle)), VLA P: VLA 1.5 GHz peak brightness, VLA I: VLA 1.5 GHz integrated flux densities. Italiscised source IDs correspond to sources with no-primary beam correction applied. The row of numbers below the column titles correspond to the columns in the machine-readable table that accompanies this paper.

(a)

Sources detected using naturally weighted taper (UVWTFN="NA" in AIPS task IMAGR).

(b)

Not primary beam corrected.

(c)

S: spectroscopic redshift, P: photometric redshift. Redshift references:

(j)

Cowie (priv. comm.)

(m)

Unknown photometric error, conservatively set to ±0:5 in calculations of derived properties.

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