Non-transiting exoplanets as a means of understanding star–planet interactions in close-in systems

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Table D.1

Candidates with an orbital period corresponding to a harmonic of the stellar rotation period

KIC	F_orb [days]	F_rot [days]	Harmonic
5560359	$1 {.96325}_{- 0.00073}^{+0 .00081}$ $\text{1}\text{.96325}_{-\text{0}\text{.00073}}^{\text{+0}\text{.00081}}$	$3 {.9}_{- 0.5}^{+0 .5}$ $\text{3}\text{.9}_{-\text{0}\text{.5}}^{\text{+0}\text{.5}}$	2
7801559	$1 {.37431}_{- 0.00051}^{+0 .00076}$ $\text{1}\text{.37431}_{-\text{0}\text{.00051}}^{\text{+0}\text{.00076}}$	$2 {.8}_{- 0.2}^{+0 .2}$ $\text{2}\text{.8}_{-\text{0}\text{.2}}^{\text{+0}\text{.2}}$	2
8193786	$2 {.18821}_{- 0.00149}^{+0 .00120}$ $\text{2}\text{.18821}_{-\text{0}\text{.00149}}^{\text{+0}\text{.00120}}$	$6 {.4}_{- 0.6}^{+0 .6}$ $\text{6}\text{.4}_{-\text{0}\text{.6}}^{\text{+0}\text{.6}}$	3

Notes. The rotation periods are taken from the catalogues by Santos et al. (2019, 2021).

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