Table 2
Results of VLBA and EVN observations.
| RA(J2000) | Dec(J2000) | Comp. | S5 GHz | θ | LAS | LLS | Tb(VLBI) | Type | ||||
| h m s | ° ′ ″ | (mJy) | (mas) | (mas) | (pc) | (109δ-1 K) | ||||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | ||||
|
|
||||||||||||
| 08 11 02.931 | 50 07 24.52 | C1 | 6.4 | 0.7 | 1.5 | 12.6 | 2.9 | CJ | ||||
| C2 | 0.8 | 0.6 | ||||||||||
| 08 42 24.395 | 06 31 16.78 | C1 | 11.5 | 1.5 | 6.8 | 55.1 | 1.3 | CJ | ||||
| C2 | 6.2 | 1.4 | ||||||||||
| C3 | 4.4 | 2.9 | ||||||||||
| 08 56 41.566 | 42 42 53.94 | C | 17.2 | 0.5 | 0.5 | 3.8 | 18.2 | S | ||||
| 10 40 59.802 | 05 55 24.78 | C1 | 1.8 | 0.8 | 2.1 | 17.0 | 0.7 | CJ | ||||
| C2 | 0.7 | 0.1 | ||||||||||
| 13 33 25.080 | 47 29 35.36 | C1 | 5.7 | 0.6 | 6.0 | 47.9 | 4.0 | CJ | ||||
| C2 | 5.1 | 1.7 | ||||||||||
| C3 | 3.3 | 0.5 | ||||||||||
| 14 01 26.163 | 52 08 34.63 | C1 | 21.4 | 0.8 | 1.2 | 9.3 | 9.6 | CJ | ||||
| C2 | 2.4 | 1.9 | ||||||||||
| 14 57 56.263 | 57 44 46.90 | C1 | 33.5 | 0.4 | 4.2 | 34.9 | 40.1 | CJ | ||||
| C2 | 7.8 | 1.6 | ||||||||||
| C3 | 7.2 | 1.9 | ||||||||||
| 21 07 57.683 | −06 20 10.49 | C | 6.7 | 0.4 | 0.4 | 2.8 | 4.8 | S | ||||
| 22 38 43.578 | 00 16 48.05 | C | 2.9 | 1.2 | 1.2 | 8.8 | 0.6 | S | ||||
| 22 48 00.717 | −09 07 44.93 | C1 | 6.6 | 1.5 | 6.0 | 49.9 | 0.6 | CJ | ||||
| C2 | 2.0 | 3.1 | ||||||||||
Notes. Description of the columns: (1) and (2) source coordinates (J2000) extracted from FIRST; (3) components as indicated on the images; (4) flux density measured with the VLBA or EVN; (5) deconvolved major axis of the Gaussian fit; (6) largest angular size (LAS) measured at 5 GHz image, LAS is defined as a separation between the two outermost Gaussian components or the size of the deconvolved component major axis (in the case of unresolved objects); (7) largest linear size (LLS) calculated based on the LAS; (8) brightness temperature calculated using Eq. (A.4); (9) suggested type of radio morphology.
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