Table 1.
Log table of our VLBI campaign and summary results of circular Gaussian fits to source visibilities.
Code | Date | Time | tobs − t0 | Array | νobs | bmaj( † ) | bmin( † ) | bp.a.( † ) | Phase Calibrator | r.m.s. ( † ) | Fν( ⋆ ) | FWHM ( ⋆ ) | ⟨βapp⟩ ( ⋆ ) |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
[hh:mm UT] | [days] | [GHz] | [mas] | [mas] | [deg] | [μJy/b] | [mJy] | [mas] | c | ||||
RG013 B | 2022-11-18 | 09:30–13:30 | 40 | EVN | 8.1–8.6 | 1.4 | 0.45 | 11 | J1905+1943 | 67 | ![]() |
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RG013 C | 2022-11-21 | 09:30–13:30 | 43 | EVN | 4.6–5.1 | 3.7 | 0.69 | 11 | J1905+1943 | 16 | ![]() |
< 0.20 | < 8.7 |
BA160 B | 2022-11-22, 23 | 19:58–00:58 | 44 | VLBA | 14.9–15.3 | 1.4 | 0.40 | −9 | J1905+1943 | 130 | ![]() |
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BA160 C | 2023-01-31 | 15:15–20:14 | 114 | VLBA | 14.9–15.3 | 1.4 | 0.58 | 3.5 | J1905+1943 | 66 | ![]() |
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RG013 D | 2023-02-03 | 05:30–11:30 | 117 | EVN | 4.6–5.1 | 7.1 | 0.9 | 7.8 | J191142+1952 | 10 | ![]() |
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RG013 E | 2023-02-04 | 05:30–11:30 | 118 | EVN | 8.1–8.6 | 1.4 | 0.59 | 10 | J191142+1952 | 21 | ![]() |
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BA160 C1 | 2023-05-02 | 10:17–15:16 | 205 | VLBA | 14.9–15.3 | 1.5 | 0.51 | −10 | J1905+1943 | 35 | ![]() |
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RG013 F | 2023-06-27, 28 | 19:30–02:36 | 261 | EVN | 4.8–5.1 | 1.8 | 1.5 | 62 | J191142+1952 | 10 | ![]() |
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BA160 D | 2023-06-28 | 04:08–09:19 | 262 | VLBA | 14.9–15.3 | 1.7 | 0.57 | −3 | J1905+1943 | 37 | ![]() |
< 9.3 | < 66 |
Notes. ( † )Beam major axis, minor axis, position angle, r.m.s. noise level with natural weights. ( ⋆ )Median and 68% confidence interval of the flux density Fν and full width at half maximum FWHM from fitting a circular Gaussian to the source visibilities; and of the average apparent expansion speed ⟨βapp⟩, assuming zero size at t0. If the lower extremum of the 68% credible interval is 0, we report the 95% upper limit instead.
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