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Table B.3.

Classification of the stationary sources identified as stars.

Source (S/N)PM (S/N)Plx u − g J − K W1 − W2 Type
GQ124804+265836 1.83 3.48 2.59 0.66 0.15 M5 star
GQ125241+275942 1.48 2.18 2.17 0.81 0.18 M5 star
GQ125543+270714 1.81 4.94 2.72 0.77 −0.11 M5 star
GQ125518+270034 1.91 1.49 2.72 0.87 0.18 M4 star
GQ124734+270615 0.89 3.86 1.87 0.73 −0.31 M4 star
GQ125050+272448 1.06 −0.62 3.10 0.89 −0.02 M4 star
GQ125159+280446 1.20 3.39 1.67 0.78 −0.09 M3 star
GQ125312+265355 1.88 0.76 3.07 0.81 0.04 M3 star
GQ125248+263805 0.69 2.20 3.21 0.88 −0.04 M3 star
GQ125308+273331 1.44 1.27 2.14 0.87 −0.50 M3 star
GQ125007+274709 0.99 2.46 2.27 0.74 0.34 M2 star
GQ125420+274609 0.76 0.96 1.85 0.78 0.10 M1 star
GQ124814+271603 0.22 1.20 2.35 0.63 −0.05 M1 star
GQ125516+265049 1.33 −0.10 3.92 0.76 M0 star
GQ124945+264953 0.63 1.39 3.78 0.73 0.20 M0 star
GQ124935+265906 1.06 1.07 3.65 0.96 −0.19 M0 star
GQ125149+265349 1.78 0.97 2.17 0.51 M0 star
GQ124715+265528 1.81 4.05 2.29 0.77 0.23 K9 star
GQ124955+275657 1.20 −1.76 1.32 0.60 0.88 K6 star
GQ124902+262014 1.44 0.28 1.72 0.66 0.46 K5 star
GQ125357+271630 1.75 0.69 2.25 −0.28 K5 star
GQ125456+263623 0.49 −0.07 2.41 0.73 −0.02 K5 star
GQ125353+273405 1.72 −1.75 1.05 0.95 −0.03 K4 star
GQ124758+272556 1.87 6.19 1.89 0.52 0.00 G8 star
GQ125158+271304 1.53 0.67 1.38 G6 star
GQ125027+263048 1.05 −0.45 1.16 0.43 G6 star
GQ124721+265728 1.19 −1.59 1.06 0.51 G6 star
GQ124922+265938 0.83 −0.86 1.20 G4 star
GQ125441+264637 1.80 −0.16 1.15 0.52 G4 star
GQ125503+264502 0.61 −1.31 1.10 0.62 G4 star
GQ124901+274330 0.91 −2.50 0.89 0.50 G0 star
GQ124959+261949 1.80 −0.31 0.94 F8 star
GQ125008+274001 1.81 −2.43 0.97 0.93 0.68 F7 star
GQ124731+270622 1.69 −1.69 0.85 F6 star
GQ124746+264709 1.87 0.52 1.01 F6 star
GQ125453+263721 1.68 −1.24 1.09 0.64 F4 star
GQ125005+280041 1.46 0.51 0.81 F4 star
GQ125134+272000 0.35 −0.78 0.94 F4 star
GQ125109+263505 1.59 −3.75 1.09 0.81 0.13 F1 star
GQ125510+263724 1.25 0.51 0.89 F0 star
GQ124820+264225 1.64 −1.26 1.06 F0 star

Notes. We have ordered the objects by the stellar classifications. 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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