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Table 2

Astrometry and photometry of CCs within the IRDIS field of view.

Star CC ID Epoch Separation PA K ΔK Status (a) pB M(b) Teff (b)
(yyyy-mm-dd) (′′) (°) (mag) (mag) (%) (M) (K)
HAT-P-41 1 2016-10-24 3.621 ± 0.004 183.9 ± 0.1 9.83 2.50 ± 0.21 C -
                     
HAT-P-57 1 2016-10-09 2.688 ± 0.004 231.8 ± 0.1 9.55 2.91 ± 0.05 C -
                     
HAT-P-57 2 2016-10-09 2.807 ± 0.004 226.9 ± 0.1 9.55 3.47 ± 0.05 C -
                     
HAT-P-57 1 2017-05-15 2.689 ± 0.004 231.8 ± 0.1 9.55 2.90 ± 0.12 C -
                     
HAT-P-57 2 2017-05-15 2.809 ± 0.004 227.0 ± 0.1 9.55 3.45 ± 0.12 C -
                     
K2-38 1 2017-03-06 1.378 ± 0.014 185.2 ± 0.6 9.47 8.72 ± 0.31 A 1.59
                     
WASP-2 1 2017-05-15 0.710 ± 0.003 104.9 ± 0.2 9.73 2.55 ± 0.07 C -
                     
WASP-7 1 2016-10-06 4.474 ± 0.007 231.5 ± 0.1 8.40 8.70 ± 0.27 B - - -
                     
WASP-8 1 2016-10-06 4.520 ± 0.005 170.9 ± 0.1 8.09 2.29 ± 0.08 C -
                     
WASP-20 1 2016-10-06 0.259 ± 0.003 216.0 ± 0.6 9.79 0.86 ± 0.06 A 0.004
                     
WASP-54 1 2017-03-05 5.728 ± 0.006 115.9 ± 0.1 9.04 5.94 ± 0.06 C -
                     
WASP-70 1 2017-05-15 3.160 ± 0.004 167.4 ± 0.1 9.85 1.38 ± 0.18 C -
                     
WASP-72 1 2017-07-06 0.639 ± 0.003 331.9 ± 0.3 9.67 3.34 ± 0.06 A 0.02
                     
WASP-76 1 2016-11-07 0.436 ± 0.003 215.9 ± 0.4 8.37 2.30 ± 0.05 C -
                     
WASP-80 1 2017-06-22 2.132 ± 0.010 275.5 ± 0.3 8.35 9.25 ± 0.28 A 3.29
                     
WASP-87 1 2017-04-02 4.109 ± 0.016 202.3 ± 0.2 9.56 8.48 ± 1.19 A 19.83
                     
WASP-87 2 2017-04-02 5.569 ± 0.007 241.0 ± 0.1 9.56 5.57 ± 0.70 B - - -
                     
WASP-88 1 2017-05-15 3.350 ± 0.015 355.5 ± 0.5 10.32 7.60 ± 0.53 A 1.65
                     
WASP-108 1 2017-03-05 0.124 ± 0.007 203.0 ± 3.3 9.83 3.90 ± 0.06 A 0.02
                     
WASP-108 2 2017-03-05 5.039 ± 0.019 174.2 ± 0.2 9.83 7.48 ± 0.43 B - - -
                     
WASP-111 1 2017-05-15 5.039 ± 0.005 100.1 ± 0.1 9.08 3.01 ± 0.17 C -
                     
WASP-118 1 2017-07-06 1.251 ± 0.004 246.5 ± 0.2 9.79 6.73 ± 0.13 A 0.09
                     
WASP-120 1 2016-12-20 2.124 ± 0.004 91.7 ± 0.1 9.95 4.44 ± 0.23 A 0.47
                     
WASP-120 2 2016-12-20 2.221 ± 0.005 89.8 ± 0.1 9.95 3.27 ± 0.32 A 0.51
                     
WASP-122 1 2016-12-25 0.837 ± 0.003 350.7 ± 0.2 9.43 5.09 ± 0.30 A 0.50
                     
WASP-123 1 2016-10-22 4.786 ± 0.005 205.0 ± 0.1 9.36 3.47 ± 0.11 C -
                     
WASP-130 1 2017-03-11 0.600 ± 0.003 98.0 ± 0.3 9.50 3.73 ± 0.12 A 0.22
                     
WASP-131 1 2017-07-05 0.189 ± 0.003 111.5 ± 0.9 8.65 2.82 ± 0.20 A 0.01
                     
WASP-137 1 2016-10-26 1.660 ± 0.003 177.0 ± 0.1 9.46 6.20 ± 0.28 A 0.14

Notes. Furthermore, we present the primary K-band magnitudes corrected for the contribution of the CCs (see Eq. (2)). (a) Status is either companion (C), background (B), or ambiguous (A). The latter classification indicates that neither the background nor the companion hypothesis are confirmed by proper motion analysis at the 5σ level. For the ambiguous cases we also present the background probability pB based on our TRILEGAL analysis (Eq. (1)) in the next column. (b) For confirmed background objects, we do not provide masses and effective temperatures because these parameters depend on the distance to the object, which is not known in these cases. For all dubious cases the distances and temperatures are calculated for the case that the object is at the same distance as the primary.

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