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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