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Table 11.

Variability index calculated between our VLBI observations and RFC observations.

Source Obs. Date ν beam Sint V
(GHz) (mas × mas,°) (mJy)
(1) (2) (3) (4) (5) (6) (7)
200109A
TXS 1100+122 RFC 30 Apr 2004 8.6 2.0 × 0.9, 1.1 311 ± 31
VLBA 04 Feb 2020 8.4 2.2 × 1.0, −6.3 409 ± 41 0.04

RFC 01 Aug 2007 8.6 2.2 × 1.2, 35.1 403 ± 41
VLBA 04 Feb 2020 8.4 2.2 × 1.0, −6.3 409 ± 41 −0.09

RFC 20 Feb 2012 8.6 2.0 × 0.9, 8.0 150 ± 15
VLBA 04 Feb 2020 8.4 2.2 × 1.0, −6.3 409 ± 41 0.38

201114A
NVSS J065844+063711 RFC 08+09 Apr 2013 4.3 4.6 × 1.9, −7.3 22.5 ± 2.4
EVN 01+02 Dec 2020 4.9 1.8 × 1.1, 82.4 12.9 ± 1.3 0.17

RFC 08+09 Apr 2013 7.6 2.8 × 1.1, −12.2 23.2 ± 2.6
VLBA 06 Dec 2020 8.4 2.0 × 1.0, 2.2 14.7 ± 1.6 0.12

RFC 19 Oct 2013 7.6 2.2 × 1.3, −3.3 15.2 ± 1.6
VLBA 06 Dec 2020 8.4 2.0 × 1.0, 2.2 14.7 ± 1.6 −0.09

Notes. Column 1: candidate neutrino counterpart; Col. 2: origin of the VLBI observation: RFC or our VLBA or EVN observations; Col. 3: date of observation; Col. 4: frequency in GHz; Col. 5: major axis (mas), minor axis (mas), and PA (in degrees, measured from north to east) of the restoring beam; Col. 6: integrated flux density in mJy; Col. 7: variability index. Negative values of V mean that the source does not show variability (Aller et al. 1992).

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