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Table 2.

Frequency-averaged polarization properties of AGN targets (at a representative frequency of 343 GHz).

Source Day Ia Spectral Index LP χ χ0 RM
(2021) (Jy) (α) (%) (deg) (deg) (105 rad m−2)
3C273 Apr 19 4.17 ± 0.42 –0.781 ± 0.008 1.67 ± 0.03 –64.19 ± 0.52 –38.9 ± 7.3 –5.8 ± 1.7
3C279 Apr 19 8.73 ± 0.87 –0.48 ± 0.04 10.63 ± 0.03 –46.711 ± 0.081 –41.2 ± 1.1 –1.26 ± 0.26
4C01.28 Apr 19 1.50 ± 0.15 –0.42 ± 0.03 8.67 ± 0.03 –37.72 ± 0.11 –37.4 ± 1.5 –0.08 ± 0.35
J1146+3958 Apr 19 0.396 ± 0.040 –0.4 ± 0.2 2.66 ± 0.07 87.27 ± 0.77 107 ± 11 –4.4 ± 2.5
J1337–1257 Apr 19 3.13 ± 0.31 –0.38 ± 0.05 16.68 ± 0.03 –7.310 ± 0.055 –8.15 ± 0.77 0.19 ± 0.18
J1512–0905 Apr 19 1.74 ± 0.17 –0.42 ± 0.04 1.07 ± 0.04 –65.72 ± 0.95 –96 ± 13 6.9 ± 3.1
M87 Apr 19 0.970 ± 0.097 –1.24 ± 0.02 2.80 ± 0.03 12.60 ± 0.35 8.5 ± 5.0 0.9 ± 1.1

non-VLBI scans
3C273b Apr 19 4.17 ± 0.42 –0.68 ± 0.01
4C01.28 Apr 19 1.50 ± 0.15 –0.36 ± 0.02 8.66 ± 0.03 –37.68 ± 0.11 –38.0 ± 1.6 0.07 ± 0.37
J1246–0730 Apr 19 0.280 ± 0.028 –0.56 ± 0.04 0.6 ± 0.1 –17.0 ± 6.6 –119 ± 95 23 ± 21

Notes.

(a)

Errors in Stokes I include thermal and 10% absolute flux systematic uncertainty summed in quadrature.

(b)

The short observation on 3C273 did not result in sufficiently good data to enable a meaningful polarization analysis.

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