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Table A.1

RHD simulation parameters.

Id Simulation M L R Teff log 𝑔 tavg Ppuls σPpuls Px Py σP σP
[M] [L] [R] [K] [cgs] [yr] [days] [days] [AU] [AU] [AU] % [R]
1 st28gm05n038 1.0 4978 281 2893 −0.46 19.05 341 31 −0.025 −0.004 0.108 8.26
2 st28gm05n043 1.0 5013 278 2908 −0.45 19.03 337 30 −0.011 −0.044 0.113 8.74
3 st28gm06n057 1.0 7055 349 2831 −0.65 15.87 485 77 0.012 0.005 0.152 9.37
4 st28gm06n059 1.0 7050 347 2837 −0.64 15.87 487 77 0.082 −0.055 0.143 8.86
5 st28gm07n006 1.0 8003 379 2801 −0.72 15.85 546 99 −0.055 0.011 0.219 12.43
6 st28gm07n008 1.0 8020 377 2812 −0.72 15.84 541 102 0.006 −0.029 0.171 9.75
7 st28gm08n001 1.0 8980 408 2780 −0.78 19.39 592 129 −0.141 −0.018 0.202 10.65
8 st29gm02n013 1.0 2983 190 3092 −0.12 11.23 178 13 −0.015 −0.012 0.052 5.89
9 st29gm03n001 1.0 3990 241 2955 −0.33 15.22 262 18 0.001 −0.001 0.094 8.39
10 st29gm03n002 1.0 4028 241 2964 −0.33 15.22 263 18 0.008 −0.008 0.133 11.87
11 st31gm01n002 1.0 2500 165 3177 0.01 9.13 134 14 −0.002 −0.003 0.028 3.65
12 st32g01n002 1.0 1978 138 3275 0.16 7.02 98 8 −0.006 −0.007 0.025 3.90

13 st28gm05n006 1.5 4985 269 2957 −0.25 15.85 240 20 −0.003 0.004 0.087 6.95
14 st28gm05n008 1.0 4942 302 2786 −0.52 15.85 387 36 0.003 −0.032 0.067 4.77
15 st28gm05n017 1.5 7490 321 2994 −0.40 15.86 328 22 −0.013 −0.072 0.129 8.64
16 st28gm05n020 1.5 7708 327 2989 −0.42 15.86 351 30 −0.046 −0.023 0.130 8.55
17 st28gm05n022 1.0 5068 312 2757 −0.55 15.85 422 42 0.005 −0.027 0.086 5.93
18 st28gm05n028 1.5 6946 306 3009 −0.36 15.85 298 16 0.028 −0.015 0.104 7.31
19 st28gm05n029 1.5 6941 288 3102 −0.31 15.70 278 15 0.024 −0.010 0.093 6.94
20 st28gm05n034 1.5 6880 278 3150 −0.28 7.93 259 14 −0.004 −0.040 0.082 6.34
21 st28gm06n032 1.0 7062 339 2872 −0.62 15.87 508 69 −0.034 0.011 0.156 9.90
22 st28gm06n043 1.0 7079 344 2854 −0.64 15.87 461 75 −0.062 −0.041 0.108 6.75
23 st28gm06n053 1.5 10073 391 2922 −0.57 15.85 418 46 0.009 −0.068 0.238 13.09

24 st26gm07n002 1.0 6986 439 2524 −0.85 25.35 594 112 −0.100(a) 0.046(a) 0.187(a) 9.16(a)
25 st26gm07n001 1.0 6953 402 2635 −0.77 27.74 517 94 −0.098(a) 0.024(a) 0.198(a) 10.59(a)
26 st28gm06n026 1.0 6955 372 2737 −0.70 25.35 471 116 −0.068(a) −0.002(a) 0.152(a) 8.79(a)
27 st29gm06n001 1.0 6995 324 2929 −0.59 31.70 389 73 −0.098(a) 0.016(a) 0.174(a) 11.55(a)
28 st27gm06n001 1.0 5011 322 2704 −0.58 31.73 450 38 −0.027 0.027 0.090 6.01
29 st28gm05n002 1.0 4978 314 2742 −0.56 25.35 393 38 −0.002(a) 0.033(a) 0.077(a) 5.27(a)
30 st28gm05n001 1.0 5019 289 2858 −0.49 31.83 360 44 −0.057 0.017 0.097 7.22
31 st29gm04n001 1.0 4982 295 2827 −0.50 25.35 339 37 −0.002(a) 0.023(a) 0.078(a) 5.69(a)

Notes. The simulations 1-12 are the new models presented in this work; the simulations 13-23 are presented in Ahmad et al. (2023) and the simulations 24-31 are presented in Freytag et al. (2017) and Chiavassa et al. (2018). The table displays the simulation name, the stellar mass M, the average emitted luminosity L, the average approximate stellar radius R, the effective temperature Teff, the surface gravity log(g), the pulsation period Ppuls, the spread in the pulsation period i.e. the pulsation period uncertainty σpuls, and the stellar time tavg used for the averaging of the rest of the quantities. The stellar parameters may slightly vary from original articles as they are updated thanks to Ahmad’s and Freytag’s work. The last four columns are the time-averaged positions Px and Py in AU and the standard deviation of the photocentre displacement σP (in AU and in % of R). Data denoted by the footnote (a) come from the previous analysis of Chiavassa et al. (2018).

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