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Table 1.

Image parameters.

Freq Obs. Code Array Date uv range Synthesized Beam Size σrms Speak Sint
Bmaj Bmin Bpa
(GHz) (dd/mm/yy) (mas) (mas) (° ) (mJy/beam) (Jy/beam) (Jy)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)
1.4 AM0672 VLA 05/11/2000 1.5–168.7 1959 1462 –85.1 0.7 2.52 2.99
5 AM0672 VLA 05/11/2000 5.1–561.2 589 447 –81.7 0.2 1.80 2.05
8.4 AH0721* VLA 12/01/2000 11.3–922.5 485 241 75.8 0.2 1.30 1.49
15 TESTT VLA 12/10/1996 14.0–1790.5 153 133 25.9 0.4 0.84 0.99
22 AH0721* VLA 12/01/2000 30.8–2452.0 175 93.5 78.8 0.3 0.73 0.88

1.7 BH065* VLBA 07/02/2000 0.9–48.0 7.51 5.60 –15.6 0.3 0.29 2.03
5 BZ061* VLBA 13/06/2016 1.7–52.4 5.41 4.89 61.1 0.2 0.16 1.14
8.4 BH096* VLBA 20/07/2002 5.5–159.1 4.59 2.88 –3.2 0.2 0.13 0.57
22 BZ061* VLBA 09/07/2016 2.3–48.0 3.42 2.71 –60.8 0.9 0.11 0.29
43 BL222* VLBA 21/06/2016 22.3–1105.4 0.47 0.31 26.7 0.9 0.016 0.017

Notes. The columns are as follows: (1) observation frequency; (2) observation code; the datasets marked with an asterisk represent our observations; (3) VLBI array used for observation; (4) observation epoch; (5) uv range of visibilities in the observational data. Notably, the uv range of the 22 GHz VLBA data was cut to get a reliable image; (6)–(8) major axis of restoring beam, minor axis of restoring beam, and position angle of major axis, respectively; (9) rms noise level of an image; (10) peak intensity of an image; (11) total flux density of an image.

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