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Table 1.

Summary of the EVN, VLBA, e-Merlin, JVLA, and LOFAR data presented in this work.

Primary data

(1) (2) (3) (4) (5) (6)
Telescope Project Code Obs. Date Time on source Frequency Calibrators
[h] [GHz]

JVLA 22A-301 May 2022 1.5 3.0 3C286, J1044+8054
0.7 5.5
2 9.0

LOFAR LC 10_010 June 2018 8 0.144 3C295, L619462

eMerlin EG080 March 28, 2014 6 1.6 0319+415, J0954+7435
March 10, 2014 6 5.0 1331+305, J0954+7435

VLBA BG 224 February 4, 2014 4 1.6 J2005+7752, J0954+7435
0.7 5.0
1.3 8.4

EVN EG080 February 26, 2014 5 1.6 3C345, J0954+7435
March 9, 2014 5 5.0

Complementary data

EVN RSG05 May 3, 2013 1 5.0 0133+476, J0954+7435
RSG07 December 1, 2015 1.5 1.6 J0958+6533, J1027+7428, J0954+7435

VLBA BE 056 July 8, 2014 0.3 5.0 4C 39.25, J1044+8054

Notes. We separate the primary, sensitive data (that we use to derive the main results) from the shorter-observing time complementary data (that we use to verify the results based on primary data). (1) Name of the radio telescope; (2) project code; (3) date of the observations; (4) time spent on the target source RBS 797; (5) observing frequency; (6) Name of the calibrators.

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