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Table B.1.

Candidate gravitationally bound companions of RR Lyrae stars. The RR subtype is taken from the VSX database (Watson et al. 2006). The references for the photometry are given in the caption of Table A.1.

RRL name / GDR2 ϖG2 μα, G2,  μδ, G2 Sep. Sep. GBP G GRP J H K W1 W2 W3 W4 E(B − V) MG Log T RR
(mas) (mas a−1) (″) (kau) type
OV And 0.9380.038 −4.900.06, −7.780.03 11.93 11.34 10.64 9.68 9.15 9.00 8.91 8.99 8.91 8.53 0.053a +1.08 3.683 RRab
380489851377596928 0.9090.039 −4.430.04, −7.710.03 3.43 3.7 13.79 13.54 13.02 +3.20 3.781 F4V

CS Del 0.6350.031 −0.320.05, +2.160.06 13.05 12.85 12.50 12.02 11.88 11.83 11.74 11.79 11.78 9.07 0.095a +1.60 3.830 RRc
1805526185917504512 0.6440.056 −0.280.10, +2.190.10 3.17 5.0 16.32 16.14 15.42 +4.93 3.774 G7V

V0893 Her 2.6790.028 −6.750.05, +11.540.06 9.33 9.16 8.84 8.45 8.32 8.26 8.25 8.26 8.22 8.02 0.022a +1.24 3.818 RR:
1385661079389302144 2.9050.443 −9.681.14, +14.081.20 5.16 1.9 16.19 16.65 15.09 +8.91 3.725 M1.5V

RR Leo 1.0320.088 −15.290.10, −10.160.10 11.12 10.91 10.48 9.92 9.68 9.64 9.63 9.63 9.58 8.25 0.037b +0.87 3.795 RRab
630421931138065280 1.0620.163 −16.300.44, −10.150.32 9.64 9.3 18.74 18.05 17.16 15.97 15.31 15.11 +8.10 3.523 M0V

SS Oct 0.8620.023 −1.900.05, −32.700.05 12.17 11.79 11.11 10.05 9.83 9.75 9.73 9.71 9.66 9.27 0.285b +0.73 3.789 RRab
6345324695303800192 0.7820.114 −2.220.32, −32.850.24 2.67 3.1 16.80 17.18 15.80 +5.90 3.797 K2V

EY Oph 0.6580.032 −2.640.06, −1.750.04 14.00 13.55 12.92 12.48 12.13 12.07 11.41 11.49 11.57 8.49 0.200a +2.12 3.769 RR:
6029835295648727168 1.5970.341 −4.520.81, −4.260.52 12.21 6.6 19.45 19.43 18.16 +9.95 3.738 M3V (WD?)

V0487 Sco 1.0690.075 −9.830.15, −12.300.12 11.54 11.22 10.67 9.90 9.65 9.60 8.14 8.20 8.30 8.67 0.252b +0.69 3.811 RRc
4053551410541112192 0.9420.060 −10.600.12, −12.610.10 29.59 27.7 16.85 15.95 14.90 12.04 10.62 10.16 9.85 9.98 9.92 8.68 +5.26 3.458 dusty M giant ?

References.

(a)

3D map Bayestar17 by Green et al. (2018);

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