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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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