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Table 3

TEP hosts with candidate companions, observing date, inferred astrometric position, and flux ratio in the observed passbands.

Name Date of obs. Sep [] PA [°] Δ i [mag] Δ z [mag] new?

CoRoT-02 21.10.2014 4.109 ± 0.025 208.56 ± 0.14 3.35 ± 0.15 3.07 ± 0.15
CoRoT-03 21.10.2014 5.221 ± 0.013 175.62 ± 0.55 3.39 ± 0.25 3.48 ± 0.36
CoRoT-11 21.10.2014 2.540 ± 0.005 307.38 ± 0.17 2.27 ± 0.09 2.14 ± 0.09
HAT-P-15 south west 21.10.2014 6.253 ± 0.026 233.42 ± 1.54 7.17 ± 0.49 6.74 ± 0.45 yes
07.03.2015 6.136 ± 0.014 235.71 ± 1.02 6.79 ± 0.22
HAT-P-15 south 07.03.2015 7.091 ± 0.014 194.23 ± 1.02 6.66 ± 0.20 yes
HAT-P-20 21.10.2014 6.925 ± 0.012 321.10 ± 0.11 2.01 ± 0.08 1.67 ± 0.08
HAT-P-24 06.03.2015 4.965 ± 0.008 171.32 ± 0.60 6.01 ± 0.18 5.80 ± 0.24
HAT-P-27/WASP-40 27.06.2013 0.656 ± 0.021 25.74 ± 1.19 yes
09.03.2015 0.644 ± 0.007 28.40 ± 1.86 4.44 ± 0.32
HAT-P-28 21.10.2014 0.972 ± 0.019 212.34 ± 2.05 6.2: 4.09 ± 0.27 yes
HAT-P-29 06.03.2015 3.276 ± 0.104 160.71 ± 1.36 7.93 ± 0.25 6.73 ± 0.35 yes
21.10.2014 3.285 ± 0.050 161.64 ± 2.36 6.31 ± 0.42 6.11 ± 0.58
HAT-P-30 09.03.2015 3.842 ± 0.007 4.25 ± 0.14 4.50 ± 0.06 4.03 ± 0.06
HAT-P-32 09.03.2015 2.930 ± 0.009 110.84 ± 0.43 5.43 ± 0.16
HAT-P-35 09.03.2015 0.933 ± 0.010 139.75 ± 1.23 5.09 ± 0.24 ⋆'° yes
HAT-P-41 21.10.2014 3.640 ± 0.011 184.00 ± 0.15 3.72 ± 0.13 3.61 ± 0.17
HAT-P-54 21.10.2014 4.531 ± 0.062 135.95 ± 1.96 5.68 ± 0.53 5.69 ± 0.59 yes
06.03.2015 4.593 ± 0.010 135.82 ± 0.27 5.61 ± 0.26
KELT-2 21.10.2014 2.402 ± 0.008 332.85 ± 0.15 3.19 ± 0.09 3.13 ± 0.09
06.03.2015 2.396 ± 0.007 332.81 ± 0.14 2.82 ± 0.15 3.02 ± 0.15
KELT-3 06.03.2015 3.762 ± 0.009 42.05 ± 0.23 3.93 ± 0.15 3.60 ± 0.15
Kepler-13 21.10.2014 1.159 ± 0.003 280.02 ± 0.22 0.24 ± 0.02 0.26 ± 0.03
Kepler-89 21.10.2014 7.316 ± 0.028 108.59 ± 0.11 3.66 ± 0.18 3.37 ± 0.23 yes
KIC10905746 21.10.2014 4.053 ± 0.007 98.61 ± 0.12 2.18 ± 0.16 1.91 ± 0.16
LHS-6343 21.10.2014 0.723 ± 0.006 119.86 ± 1.30 2.29 ± 0.24 1.66 ± 0.13
TrES-4 07.03.2015 1.583 ± 0.019 0.69 ± 0.31 4.06 ± 0.07 4.04 ± 0.09
WASP-11 21.10.2014 0.374 ± 0.013 219.75 ± 0.79 2.94 ± 0.50 2.93 ± 0.45
06.03.2015 0.383 ± 0.033 218.33 ± 1.41 3.18 ± 0.26 2.91 ± 0.20
WASP-12 06.03.2015 1.078 ± 0.008 250.08 ± 0.55 4.13 ± 0.10 3.68 ± 0.08
WASP-14 06.03.2015 1.425 ± 0.024 102.39 ± 0.40 7.14 ± 0.22 5.95 ± 0.10
WASP-33 21.10.2014 1.920 ± 0.012 275.87 ± 0.71 9.7: 7.23 ± 0.22
WASP-36 09.03.2015 4.845 ± 0.017 67.23 ± 0.95 8.5: 6.45 ± 0.59
WASP-56 06.03.2015 3.424 ± 0.009 113.35 ± 0.18 6.85 ± 0.24 5.95 ± 0.22 yes
WASP-70 21.10.2014 3.195 ± 0.029 167.83 ± 0.19 2.62 ± 0.18 2.49 ± 0.20
WASP-76 21.10.2014 0.425 ± 0.012 216.90 ± 2.93 2.51 ± 0.25 2.85 ± 0.33 yes
WASP-77 21.10.2014 3.282 ± 0.007 154.02 ± 0.12 1.80 ± 0.06 1.63 ± 0.06
WASP-85 09.03.2015 1.470 ± 0.003 100.09 ± 0.19 0.89 ± 0.01 0.85 ± 0.01
WASP-103 07.03.2015 0.242 ± 0.016 132.66 ± 2.74 3.11 ± 0.46 2.59 ± 0.35 yes
XO-3 06.03.2015 6.078 ± 0.081 297.21 ± 0.13 8.13 ± 0.28 7.93 ± 0.25

Notes. In the last column we indicate whether the companion was announced previously. No observation in this band.

(⋆)

Companion candidate was too weak for flux measurement.

(†)

The source was not identified first by us (Wöllert et al. 2015), but it could be located after the new observation with better contrast.

(°)

The exposure time in z was five times shorter than the one in i.

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