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Table 1.

Polarization and variability properties for the sources included in this study.

RBPL ID Alt. ID Π (%) Ψ (deg) Ntot Nvar Πvar Ψvar Cad. (min) Π1/η Ψ1/η
J0211+1051 CGRaBS J0211+1051 8.0 ± 2.7 76.8 ± 3.3 5 4 Y Y 2.17 2 ± 1 1.4 ± 0.3
J0217+0837 CGRaBS J0217+0837 14.0 ± 2.4 66.2 ± 3.1 7 4 Y Y 2.67 0.6 ± 0.6 0.5 ± 0.7
J0958+6533 S4 0954+65 6.82 ± 0.54 1.8 ± 4.2 1 1 Y Y 5.20 0.7 1.4
J1037+5711 GB6 J1037+5711 9.0 ± 2.4 32.3 ± 4.2 2 0 N N 3.17 0.8 ± 0.5 0.44 ± 0.01
J1058+5628 TXS 1055+567 2.86 ± 0.65 −0.4 ± 7.4 1 0 N N 7.06 0.5 0.5
J1248+5820 TXS 1246+586 5.5 ± 1.0 −77 ± 34 5 0 N N 3.17 0.4 ± 0.1 0.5 ± 0.3
J1512-0905 PKS 1510-089 3.15 ± 0.81 6 ± 94 1 1 N Y 2.17 0.6 3.3
J1542+6129 GB6 J1542+6129 3.9 ± 1.5 0.1 ± 4.7 3 0 N N 2.17 0.6 ± 0.1 0.5 ± 0.2
J1748+7005 S5 1749+70 6.09 ± 0.94 −62.0 ± 8.0 3 1 N Y 1.83 0.58 ± 0.04 0.57 ± 0.06
J1754+3212 RGB J1754+322 2.35 ± 0.81 36 ± 34 3 1 Y Y 3.43 0.4 ± 0.3 0.6 ± 0.2
J1800+7828 S5 1803+78 5.55 ± 0.99 89.0 ± 7.5 1 1 N Y 3.35 0.70 0.70
J1806+6949 S4 1807+69 8.34 ± 0.89 64.8 ± 1.7 3 3 Y Y 1.50 0.59 ± 0.05 0.6 ± 0.1
J1903+5540 TXS 1902+556 6.7 ± 1.2 35.0 ± 4.0 7 4 Y Y 3.58 0.67 ± 0.08 0.5 ± 0.1
J2005+7752 S5 2007+77 5.9 ± 1.6 −75.2 ± 5.1 2 2 Y Y 3.17 0.8 ± 0.2 0.6 ± 0.2
J2030-0622 TXS 2027-065 1.02 ± 0.36 −44 ± 21 2 1 N Y 6.83 0.8 ± 0.4 0.6 ± 0.2
J2143+1743 S3 2141+17 1.51 ± 0.49 −48 ± 13 1 1 Y Y 6.43 0.8 0.6
J2148+0657 4C+06.69 2.2 ± 1.5 −32 ± 71 7 4 Y Y 6.82 0.7 ± 0.1 0.5 ± 0.2
J2202+4216 BL Lacertae 7.0 ± 4.2 55 ± 30 7 5 Y Y 5.65 1 ± 1 1 ± 3
J2232+1143 CTA 102 3.2 ± 3.3 −85 ± 83 3 2 Y Y 2.68 0.9 ± 0.8 0.7 ± 0.2
J2253+1608 3C 454.3 3.33 ± 0.98 89.4 ± 6.3 2 2 Y Y 3.17 0.9 ± 0.2 0.80 ± 0.05

Notes. The first two columns list the RoboPol ID and alternative source names. The third and fourth columns give the median polarization degree (Π) and polarization angle (Ψ) across all observations of each source presented here averaged in the Stokes Q-U space. The polarization angles are modified with the π ambiguity so that all the values in the column are between −90 and 90 degrees. Columns Ntot and Nvar report the total number of nights observed and the number of nights when variability was detected, respectively. In the Πvar and Ψvar columns, a Y indicates that variability was detected in Π or Ψ. The next column shows the average cadence for each source, i.e., the median time interval between two consecutive observations, and the last two columns show the median value and its standard deviation for the 1/η metric for Π and Ψ, respectively.

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