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Table A.1

CORALIE radial velocities of EBLM J0555-57A, and the probability that a point is not contaminated by the blend star.

BJD – 2 400 000 RV 1σ FWHM Bisector span Depth of normalized CCF Probability Spectrum rejected
day km s-1 km s-1 km s-1 km s-1 %

56 610.686754 25.078 0.012 14.179 0.310 17.149 0.000 x
56 615.797803 20.914 0.014 13.039 0.242 18.309 0.000 x
56 629.624924 13.125 0.018 14.624 0.101 16.583 0.000 x
56 640.778888 25.616 0.022 14.974 0.621 16.129 0.000 x
56 641.641065 25.229 0.020 14.362 0.424 16.560 0.000 x
56 644.700696 12.230 0.022 15.307 0.262 15.542 0.000 x
56 695.539666 26.056 0.021 14.697 0.215 16.161 0.000 x
56 697.572545 16.661 0.022 13.917 –0.463 16.930 N/A xa
56 715.565737 15.302 0.014 13.869 –0.056 17.264 0.560
56 716.588522 20.783 0.014 13.690 0.069 17.392 0.082
56 717.511413 24.949 0.023 13.837 0.071 16.637 0.873
56 718.547982 26.902 0.023 13.938 0.081 16.731 0.183
56 719.534391 24.542 0.023 13.828 0.215 16.913 0.962
56 723.625576 17.069 0.018 13.624 –0.201 17.246 0.013
56 739.593653 19.399 0.015 13.797 0.012 16.991 0.726
56 740.590941 24.250 0.017 13.809 0.051 16.914 0.847
56 744.513089 13.487 0.020 13.866 0.073 16.544 0.610
56 746.538624 15.208 0.021 13.870 –0.086 16.822 0.577
56 770.473218 19.968 0.021 9.1723 0.021 26.673 N/A x b
56 770.488252 18.650 0.020 13.668 –0.045 17.040 0.059
57 082.579230 25.648 0.032 14.406 0.309 17.435 0.000 x
57 085.612435 14.950 0.023 13.866 –0.022 18.013 0.618
57 086.640474 11.384 0.022 14.154 0.338 17.643 0.000 x
57 117.510586 11.564 0.032 14.182 0.158 17.501 0.000 x
57 400.680862 26.035 0.030 14.424 0.260 17.408 0.000 x
57 417.703102 24.652 0.025 13.768 0.079 18.222 0.527
57 420.648080 11.791 0.021 13.786 0.113 18.130 0.648
57 422.573335 21.016 0.026 13.674 0.067 18.352 0.090
57 772.591031 25.051 0.035 13.850 0.086 18.070 0.797
57 773.731230 26.807 0.025 13.916 0.000 17.930 0.296
57 774.695330 23.836 0.033 13.777 0.216 18.015 0.626

Notes. The radial velocity data are seperated into two sets, before and after tJDB−2,400,000 = 56 770.48, to account for an upgrade of the instrument (Triaud et al. 2017). Separate systemic velocities are used for each set, determining γ1 = 19.537 ± 0.015 km s-1, γ2 = 19.491 ± 0.008 km s-1. All times are given in the BJDUTC timestamp.

(a)

Rejected before the FWHM outlier analysis due to anomalous span of the bisector inverse slope.

(b)

Spectrum of EBLM J0555-57B

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