Table 6.
Image parameters.
Source (J2000) | Obs | S86 GHz | SS | BS | SL | BL | Ba | Bb | BPA | St | Sp | σ | ξr |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) | (13) | (14) |
J0013+4051 | C | 0.79 | 0.656 ± 0.020 | 56 | 0.192 ± 0.006 | 3136 | 159 | 35 | −16.8 | 436 | 317 | 8 | 1.43 |
J0017+8135 | B | 0.18 | 0.263 ± 0.018 | 60 | 0.075 ± 0.004 | 3062 | 74 | 35 | 62.1 | 143 | 81 | 2 | 1.36 |
J0030+7037 | B | 0.34 | 0.363 ± 0.026 | 65 | 0.115 ± 0.009 | 3070 | 76 | 36 | 66.5 | 155 | 92 | 3 | 1.34 |
J0034+2754 | C | 0.07 | 0.124 ± 0.015 | 54 | 0.156 ± 0.021 | 3086 | 262 | 36 | −14.2 | 159 | 60 | 2 | 1.04 |
J0044+6803 | B | 0.17 | 0.315 ± 0.023 | 65 | 0.097 ± 0.006 | 3034 | 75 | 36 | 70.4 | 133 | 99 | 3 | 1.15 |
J0046+2456 | A | 0.47 | 0.252 ± 0.019 | 59 | 0.137 ± 0.009 | 3060 | 267 | 37 | −15.0 | 235 | 160 | 6 | 1.17 |
J0057+3021 | A | 0.48 | 0.361 ± 0.023 | 58 | 0.233 ± 0.017 | 3060 | 308 | 37 | −14.5 | 306 | 226 | 8 | 1.07 |
J0102+5824 | B | 3.11 | 3.579 ± 0.037 | 44 | 0.336 ± 0.020 | 3050 | 59 | 43 | −19.5 | 2221 | 1075 | 19 | 1.58 |
J0109+6133 | B | 0.64 | 0.706 ± 0.026 | 45 | 0.242 ± 0.023 | 3048 | 111 | 37 | −12.9 | 381 | 239 | 5 | 1.17 |
J0112+3522 | A | 0.53 | 0.624 ± 0.031 | 58 | 0.105 ± 0.008 | 3054 | 205 | 37 | −18.3 | 238 | 119 | 3 | 1.08 |
J0113+4948 | A | 0.61 | 0.547 ± 0.026 | 56 | 0.156 ± 0.011 | 3066 | 119 | 36 | −28.2 | 269 | 234 | 9 | 1.32 |
J0126+7046 | B | 0.07 | 0.233 ± 0.018 | 48 | 0.071 ± 0.004 | 2474 | 115 | 36 | −13.4 | 76 | 69 | 2 | 1.20 |
J0136+4751 | B | 1.95 | 2.531 ± 0.060 | 33 | 1.324 ± 0.037 | 2388 | 157 | 43 | −14.4 | 2090 | 862 | 14 | 1.21 |
J0136+4751 | C | 1.76 | 1.811 ± 0.026 | 46 | 0.518 ± 0.045 | 2870 | 230 | 36 | −0.5 | 1317 | 740 | 15 | 1.15 |
J0137+2145 | A | 0.07 | 0.289 ± 0.018 | 54 | 0.184 ± 0.007 | 3070 | 259 | 40 | −10.2 | 278 | 175 | 3 | 1.03 |
J0154+4743 | B | … | 0.436 ± 0.022 | 32 | 0.315 ± 0.026 | 2860 | 150 | 42 | −11.2 | 239 | 172 | 4 | 1.12 |
J0205+3212 | A | 0.81 | 0.530 ± 0.037 | 49 | 0.228 ± 0.019 | 3052 | 185 | 38 | −11.6 | 499 | 182 | 4 | 1.09 |
J0253+3217 | A | 0.37 | 0.579 ± 0.032 | 43 | 0.276 ± 0.014 | 3070 | 190 | 39 | −9.0 | 259 | 205 | 5 | 1.01 |
J0254+2343 | A | 0.05 | 0.342 ± 0.035 | 48 | 0.340 ± 0.027 | 3060 | 245 | 39 | −8.7 | 186 | 170 | 5 | 0.99 |
J0310+3814 | B | 0.44 | 0.320 ± 0.017 | 58 | 0.272 ± 0.021 | 3050 | 193 | 40 | −29.3 | 190 | 182 | 9 | 1.35 |
J0313+4120 | B | 0.89 | 0.823 ± 0.031 | 58 | 0.294 ± 0.018 | 3020 | 178 | 39 | −30.9 | 663 | 349 | 8 | 1.26 |
J0319+4130 | A | 12.06 | 4.690 ± 0.181 | 26 | 0.506 ± 0.054 | 3064 | 155 | 33 | −12.2 | 7677 | 978 | 10 | 1.16 |
J0319+4130 | B | 12.15 | 9.885 ± 0.206 | 55 | 0.357 ± 0.074 | 2972 | 170 | 44 | −24.1 | 8865 | 724 | 9 | 1.12 |
J0319+4130 | C | 13.85 | 3.290 ± 0.126 | 67 | 0.158 ± 0.017 | 1634 | 185 | 116 | 2.7 | 3504 | 625 | 6 | 0.66 |
J0325+2224 | C | 0.90 | 0.879 ± 0.037 | 39 | 0.266 ± 0.010 | 3131 | 203 | 37 | −9.0 | 621 | 370 | 12 | 1.12 |
J0325+4655 | C | 0.27 | 0.258 ± 0.018 | 33 | 0.074 ± 0.008 | 3135 | 127 | 40 | −9.3 | 190 | 88 | 4 | 0.81 |
J0333+6536 | C | 0.07 | 0.189 ± 0.020 | 40 | 0.158 ± 0.013 | 3050 | 109 | 37 | −12.0 | 77 | 64 | 3 | 1.04 |
J0344+6827 | A | 0.06 | 0.187 ± 0.023 | 62 | 0.136 ± 0.007 | 3138 | 122 | 39 | −35.5 | 105 | 97 | 3 | 1.10 |
Notes. Columns: (1) – IAU source name (J2000); (2) – observing epochs – A: October 2010; B: May 2011 and C: October 2011; (3) – total single dish flux density measured at 86 GHz obtained from the pointing and calibration scan measurements at Pico Veleta or Plateau de Bure (Jy); (4),(6) – correlated flux densities (Jy) measured on projected baseline lengths listed in Cols. (5) and (7) (Mλ); (8) – major axis of the restoring beam (μas); (9) – minor axis of the restoring beam (μas); (10) – position angle of the major axis (degrees); (11) – total clean flux density (mJy); (12) – peak flux density (mJy beam−1); (13) – off-source rms noise in the residual image (mJy beam−1); (14) – quality factor of the residual noise in the image. The full table is available at the CDS and in a machine-readable and Virtual Observatory (VO) forms in the online journal.
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