Planet-star interactions with precise transit timing - IV. Probing the regime of dynamical tides for GK host stars

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Table B.5

Spectroscopic parameters for the host stars, taken from the literature as the inputs in this study.

Star	T_eff (K)	log ɡ_✶ (cgs)	[Fe/H]	Source	K_b (m s⁻¹)	Source
HATS-18	5600 ± 120	…^a	0.28 ± 0.08	Penev et al. (2016)	415.2 ± 10.0	Penev et al. (2016)
HIP 65A	4590 ± 49	…^a	0.18 ± 0.08	Nielsen et al. (2020)	753.7 ± 5.0	Nielsen et al. (2020)
TrES-3	5650 ± 75	4.4 ± 0.1	−0.19 ± 0.08	Sozzetti et al. (2009)	348.5 ± 4.9	Bonomo et al. (2017)
WASP-19	5500 ± 100	4.5 ± 0.2	0.02 ± 0.09	Hebb et al. (2010)	257.9 ± 2.9	Bonomo et al. (2017)
WASP-43	4400 ± 200	4.5 ± 0.2	−0.05 ± 0.17	Hellier et al. (2011a)	549.5 ± 3.8	Davoudi et al. (2021)
WASP-173A	5700 ± 150	4.5 ± 0.2	0.16 ± 0.14	Hellier et al. (2019)	645 ± 7	Hellier et al. (2019)

Notes. T_eff is the effective temperature. log ɡ_✶ is the gravity acceleration at the bottom of the photosphere. [Fe/H] is the metallicity. K_b is the amplitude of the reflex RV induced by the hot Jupiter companion.

^a A value from pure spectroscopic analysis is not provided in the source paper.

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