Table B.2.
Classification of the stationary sources identified as quasars.
| Source | (S/N)μ | (S/N)plx | u − g | J − K | W1 − W2 | zprev. | zthis work | AV (mag) | Survey |
|---|---|---|---|---|---|---|---|---|---|
| GQ125005+263107 | 0.63 | 0.19 | −0.04 | 0.98 | 1.06 | 2.044 | – | 0.00 | SDSS |
| GQ125219+264053 | 1.07 | 1.56 | – | – | – | 1.287 | – | −0.05 | SDSS |
| GQ125209+265018 | 1.17 | −0.96 | 1.51 | – | 0.59 | 3.441 | – | 0.03 | SDSS |
| GQ125358+262453 | 0.49 | −1.48 | 0.75 | – | 0.87 | 3.100 | – | −0.02 | SDSS |
| GQ125302+270519 | 1.67 | −1.15 | 2.18 | 1.00 | 0.83 | 2.988 | – | −0.05 | SDSS |
| GQ125019+274443 | 1.75 | 0.02 | 0.84 | 1.47 | 1.03 | 2.665 | – | 0.31 | SDSS |
| GQ124816+265235 | 1.05 | −1.78 | 0.62 | 1.19 | 0.72 | 2.514 | – | −0.07 | SDSS |
| GQ125202+275018 | 0.66 | 0.80 | 0.53 | 1.32 | 1.16 | 2.485 | – | 0.04 | SDSS |
| GQ125302+261711 | 0.46 | −0.05 | 0.59 | 1.50 | 0.44 | 2.316 | – | −0.07 | SDSS |
| GQ125257+274542 | 1.61 | 1.26 | 0.31 | 0.89 | 1.37 | 2.004 | – | −0.08 | SDSS |
| GQ125150+263900 | 0.86 | 0.39 | 0.12 | 0.92 | 0.92 | 1.913 | – | 0.19 | SDSS |
| GQ125039+272904 | 1.16 | −0.85 | 0.60 | 1.23 | 1.19 | 1.890 | – | 0.37 | SDSS |
| GQ124816+264712 | 0.60 | 1.08 | −0.04 | 0.94 | 1.37 | 1.856 | – | −0.03 | SDSS |
| GQ124943+261629 | 0.53 | 0.36 | 0.05 | 0.90 | 0.11 | 1.843 | – | 0.02 | SDSS |
| GQ125015+264337 | 0.21 | −0.85 | 0.06 | 1.09 | 1.46 | 1.787 | – | −0.10 | SDSS |
| GQ125206+272717 | 1.69 | −1.63 | 0.07 | 0.84 | 1.23 | 1.680 | – | −0.04 | SDSS |
| GQ125429+270003 | 1.25 | 1.61 | 0.19 | 1.11 | 1.25 | 1.635 | – | −0.07 | SDSS |
| GQ125332+272225 | 1.69 | 0.87 | 0.27 | – | 1.32 | 1.627 | – | −0.11 | SDSS |
| GQ125424+263941 | 1.19 | −0.64 | 0.23 | 1.08 | 1.57 | 1.601 | – | −0.17 | SDSS |
| GQ124846+271722 | 0.79 | −1.43 | 0.36 | 1.07 | 1.35 | 1.514 | – | 0.21 | SDSS |
| GQ125023+265328 | 0.21 | −0.23 | 0.36 | 1.09 | 1.10 | 1.490 | – | 0.02 | SDSS |
| GQ125300+271234 | 1.16 | −0.31 | 0.26 | 1.03 | 1.44 | 1.482 | – | −0.12 | SDSS |
| GQ125302+262722 | 1.26 | 3.30 | 0.21 | 1.36 | 1.25 | 1.259 | – | −0.06 | SDSS |
| GQ124925+272634 | 0.55 | −0.55 | 0.13 | 1.41 | 1.41 | 1.156 | – | −0.11 | SDSS |
| GQ125320+270607 | 0.40 | −0.24 | 0.42 | 1.36 | 1.39 | 1.153 | – | 0.21 | SDSS |
| GQ125112+275222 | 0.38 | −0.26 | 0.19 | 1.12 | 1.30 | 1.044 | – | −0.05 | SDSS |
| GQ125528+271330 | 0.73 | −1.45 | 0.15 | 1.42 | 1.30 | 1.026 | – | −0.12 | SDSS |
| GQ124752+273018 | 1.37 | 0.63 | 0.39 | 1.23 | 0.70 | 0.914 | – | 0.10 | SDSS |
| GQ124725+270114 | 0.63 | −0.36 | 0.45 | 1.23 | 1.04 | 0.804 | – | 0.01 | SDSS |
| GQ124926+264101 | 0.64 | 0.09 | 0.43 | 1.28 | 1.09 | 0.667 | – | 0.07 | SDSS |
| GQ124832+265312 | 1.14 | 0.72 | 0.41 | 1.92 | 1.09 | 0.585 | – | −0.10 | SDSS |
| GQ125320+272116 | 0.59 | 0.89 | 0.25 | 1.50 | 1.03 | 0.512 | – | −0.14 | SDSS |
| GQ125126+261346 | 1.14 | −1.63 | −0.03 | 0.79 | 1.23 | 1.430 | 1.432 | −0.03 | CFHT |
| GQ125006+265939 | 0.63 | 0.82 | 0.11 | 1.15 | 1.20 | 0.970 | 0.980 | 0.00 | CFHT |
| GQ124915+274554 | 0.95 | 0.40 | 0.24 | 1.21 | 1.55 | 2.16P | 2.160 | −0.03 | This work |
| GQ125239+280127 | 1.96 | 1.63 | 0.06 | 1.03 | 1.31 | 2.04P | 2.070 | 0.03 | This work |
| GQ125211+272803 | 0.63 | −1.18 | 0.08 | 1.39 | 1.06 | 1.87P | 2.044 | −0.08 | This work |
| GQ125241+272550 | 1.87 | −1.36 | 0.16 | 1.16 | 1.37 | 0.22P | 2.000 | 0.28 | This work |
| GQ124958+275703 | 0.49 | 0.66 | 0.23 | 0.99 | 1.33 | 1.91P | 1.960 | 0.03 | This work |
| GQ124958+273317 | 0.48 | −0.48 | 0.15 | 0.69 | 1.51 | 1.72P | 1.950 | −0.05 | This work |
| GQ124728+272742 | 1.28 | 1.60 | 0.58 | 1.15 | – | 0.46P | 1.840 | 0.01 | This work |
| GQ125054+264353 | 1.67 | 0.85 | 0.39 | 2.17 | 1.36 | 1.59P | 1.760 | 0.04 | This work |
| GQ125327+273733 | 1.32 | 1.65 | 0.07 | 0.24 | 1.03 | 1.96P | 1.700 | −0.11 | This work |
| GQ125359+272014 | 1.09 | 1.72 | 0.26 | – | 1.55 | 0.08P | 1.700 | −0.09 | This work |
| GQ124955+271335 | 0.92 | −0.18 | 0.05 | 1.11 | 1.46 | 1.47P | 1.500 | −0.18 | This work |
| GQ125033+274519 | 0.55 | −1.24 | 0.12 | 1.72 | 1.44 | 1.48P | 1.485 | −0.07 | This work |
| GQ125424+264833 | 0.84 | 0.46 | 0.20 | – | 1.36 | 1.47P | 1.470 | −0.17 | This work |
| GQ125042+274012 | 0.16 | −1.19 | 0.21 | 1.04 | 1.44 | 1.48P | 1.455 | 0.01 | This work |
| GQ125013+273256 | 0.85 | −2.01 | 0.09 | 1.28 | 1.32 | 1.15P | 1.423 | −0.02 | This work |
| GQ125104+273341 | 0.46 | 0.38 | 0.02 | 1.48 | 1.28 | 1.15P | 1.320 | 0.00 | This work |
| GQ125133+264550 | 1.16 | −0.19 | 0.12 | 1.62 | 1.43 | 1.28P | 1.280 | −0.04 | This work |
| GQ125421+265454 | 0.15 | −2.05 | 0.21 | 1.53 | 1.22 | 1.30P | 1.266 | 0.07 | This work |
| GQ125230+275410 | 1.66 | −0.73 | 0.11 | 1.87 | 1.05 | 1.04P | 1.250 | −0.06 | This work |
| GQ124835+263759 | 1.29 | −1.23 | 0.03 | 1.26 | 1.18 | 1.15P | 1.225 | −0.03 | This work |
| GQ124809+271650 | 0.32 | −0.69 | 0.24 | 1.33 | 1.16 | 0.95P | 1.017 | 0.01 | This work |
| GQ125312+275524 | 1.80 | 2.45 | 0.23 | 0.95 | 1.26 | 1.00P | 0.980 | −0.01 | This work |
| GQ125249+280356 | 0.15 | 0.62 | 0.11 | 1.16 | 1.07 | 0.93P | 0.944 | −0.10 | This work |
| GQ125043+271934 | 1.29 | −0.81 | 0.12 | 1.62 | 0.84 | 0.93P | 0.924 | −0.17 | This work |
| GQ125107+271451 | 0.90 | −0.55 | 0.40 | 1.04 | 0.72 | 0.38P | 0.930 | 0.42 | This work |
| GQ125031+261953 | 0.28 | −1.37 | 0.22 | 1.22 | 1.06 | 0.88P | 0.860 | −0.14 | This work |
| GQ124941+265314 | 0.45 | 0.05 | 0.62 | 1.49 | 0.69 | 2.46P | 0.750 | −0.02 | This work |
| GQ125008+263658 | 0.93 | 0.32 | 0.39 | 1.44 | 1.04 | 0.68P | 0.678 | −0.07 | This work |
| GQ124921+264446 | 0.33 | −1.08 | 0.01 | 1.89 | 1.02 | 0.31P | 0.300 | 0.19 | This work |
Notes. We have ordered the sources by redshift and separated the quasars that were observed spectroscopically by previous surveys and this work. The redshifts from the SDSS archive is from the most recent DR14Q compilation (Pâris et al. 2018) and the redshifts from the CFHT survey are from Crampton et al. (1987). For the objects identified as quasars as part of this work, we also provide the photometric redshifts from Richards et al. (2009). We include measurements of the signal-to-noise of the proper motions and parallaxes as reported in the Gaia-DR2 catalogue and the typical optical, NIR, and MIR colours used to identify quasars.
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