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Table 1

Data used in this study (first ten rows; the full table is available at CDS).

IERS OR offsets Spectral γ flux Position error


name Avar mas Fvar Total mas Norm G BP-RP class ×10−10 photon cm−2 s−1 z VLBI mas Gaia mas
0002−478 0.680 0.128 0.212 0.771 19.623 0.708 FSRQ 4.6 0.880 0.109 0.255
0003−066 0.348 0.119 0.152 2.027 17.231 1.296 FSRQ 1.2 0.347 0.032 0.088
0007+106 0.211 0.101 0.315 5.191 15.863 0.944 FSRQ 0.087 0.039 0.048
0007+171 0.715 0.050 0.927 11.249 16.823 0.341 FSRQ 1.601 0.072 0.071
0008−264 0.412 0.036 0.288 1.455 18.901 0.528 QSO 1.096 0.038 0.203
0009−148 1.134 0.562 1.235 2.005 19.661 0.926 FSRQ 0.260 0.784
0013−005 0.340 0.073 0.908 3.564 19.629 0.997 FSRQ 3.5 1.576 0.059 0.371
0014+813 0.267 0.025 0.283 6.158 15.931 0.865 FSRQ 3.366 0.031 0.035
0016+731 0.194 0.151 0.211 1.840 17.725 0.783 FSRQ 8.2 1.781 0.031 0.110

Notes. (1) IERS B1950 designation, (2) astrometric variability, (3) Gaia fractional variability, (4) total optical-radio offsets between Gaia and ICRF3 and (5) associated normalized offsets, (6) Gaia G magnitude, (7) Gaia BP-RP, (8) spectral class from NED, (9) γ 1–100 Gev flux of photons per square centimeter per second from Fermi-LAT 4FGL DR3, (10) redshift from NED, (11) VLBI (ICRF3) astrometric precision, and (12) Gaia DR3 astrometric precision. In the full table, the spectral classes are coded by numerical values: 0 for FSRQ, 1 for QSO, 2 for BL Lac, 3 for Seyfert 1, 4 for Seyfert 2, 5 for GPS, 6 for CSS, 7 for other, and not-a-number if still undetermined.

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