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Table 2.

Summary of the radio observations.

Radio Project Target ν Δν Observation Duration Primary
telescope code name (MHz) (MHz) date (min) calibrators
GMRT 19043 R14D23 150 16 (14) 2011 Jan. 24 15 3C48, 3C286
GMRT 19043 R14D24 150 16 (14) 2011 Jan. 24 15 3C48, 3C286
GMRT 19043 R14D25 150 16 (14) 2011 Jan. 24 15 3C48, 3C286
GMRT 17073 A496 330 16 (11) 2010 Jan. 15 124 3C48, 3C286
GMRT 05DAG01 A496 617 32 (30) 2004 Mar. 22 78 3C48
VLITE–A 20B-138 (a) A496 340 64 (38) 2021 Feb. 15 102 3C48, 3C147, 3C286
VLA–B AC540 0434−131 1365/1465 25/25 2000 Jan. 04 147 3C138, 3C147
VLA–B AC540 0434−131 1365/1465 25/25 2000 Jan. 07 147 3C138, 3C147
VLA–A AC572 0431−132 1465/1515 25/25 2000 Dec. 13 113 3C286
VLA–A A074 A496 4835/4885 50/50 1987 Sep. 22 9 3C138
VLA–B AB398 A496 4823/4873 25/25 1986 Sep. 07 8 3C286
VLA–C AC572 0431−1321 4535/4885 50/50 2001 Jun. 21 90 3C48
VLA–D AS220 A496 4835/4885 50/50 1985 Dec. 18 20 3C285

Notes. Column 1: radio telescope (the array configuration is reported for the VLA and VLITE). Column 2: project code. Column 3: target name. Columns 4–5: observing frequency and bandwidth. For the VLA observations, we report the frequency and bandwidth of the two intermediate frequency channels. For the GMRT and VLITE datasets, the usable bandwidth after data flagging is reported in parentheses. Columns 6–7: observing date and time. Column 8: calibration sources used to set the flux density scale (see text for details).

(a)

Primary VLA project during which VLITE was operational.

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