Table 1
Fifteen target sources in the EVN experiment described in this paper.
| Source name | RA (J2000) | Dec (J2000) | Flux density | |
| h m s | ° ′ ″ | mJy | ||
|
|
||||
| FIRST-6 | 22 28 42.206 | 01 14 47.73 | 1.06 | |
| J2228+0110* | 22 28 43.540 | 01 10 32.22 | 1.32 | |
| VLA-5* | 22 28 49.842 | 01 13 37.47 | 1.76 | |
| NVSS-1 | 22 28 51.380 | 01 07 09.40 | 2.5 | |
| VLA-4* | 22 28 51.452 | 01 12 03.39 | 0.37 | |
| NVSS-2 | 22 29 00.420 | 01 17 46.90 | 2.7 | |
| VLA-3* | 22 29 18.059 | 01 06 18.43 | 7.97 | |
| VLA-1* | 22 29 18.689 | 01 09 03.09 | 1.44 | |
| VLA-2* | 22 29 25.487 | 01 17 52.61 | 0.43 | |
| FIRST-1 | 22 29 31.387 | 01 14 43.99 | 0.90 | |
| FIRST-2 | 22 29 33.802 | 01 15 38.08 | 2.02 | |
| FIRST-4 | 22 29 38.594 | 01 17 34.96 | 1.02 | |
| NVSS-3 | 22 29 38.790 | 01 18 05.20 | 3.1 | |
| FIRST-3 | 22 29 41.761 | 01 14 28.46 | 2.07 | |
| FIRST-5 | 22 29 52.917 | 01 12 19.57 | 0.92 | |
Notes. Columns 2–3: a priori right ascension (RA) and declination (Dec) in the J2000 equatorial coordinate system, which were used for the correlation; the coordinates of the sources marked with an asterisk are from the Stripe 82 VLA Survey (Hodge et al. 2011); the rest are from the FIRST (White et al. 1997) and NVSS (Condon et al. 1998) surveys, as indicated by the source names; Col. 4: the integrated flux density of each source at 1.4 GHz measured in the respective low-resolution VLA observations mentioned above.
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