Table D.1
RV variability and periodicities in RV and TESS data
| Name | N(RV)a | rmsRVb [m s−1] | m′10dk [MJup] | P1(RV)c [d (FAP)] | P2(RV) [d (FAP)] | N(TESS) Sectors | Pl(TESS)d [d (power)] | P2(TESS) [d (power)] | P3(TESS) [d (power)] | Prote [d] | Notesg |
|---|---|---|---|---|---|---|---|---|---|---|---|
| HD 105 | 16 | 40.7 | 1.7 | 1.5 (<0.001) | 2.9 (0.005) | 2 | 2.95 (0.82) | – | – | 2.95±0.1 | 1, 10 |
| HD 377i | 10 | 62.9f | 2.4 | (1.8 (0.3)) | (3.8 (0.5)) | 2 | 1.80 (0.46) | 3.61 (0.28) | – | 3.6±0.1 | 2, 11 |
| HD 870i | 16 | 5.8 | 0.2 | – | – | 4 | 5.7 (0.7) | 9.7 (0.44) | 3.8 (0.08) | 10±1 | 2 |
| HD 1466i | 16 | 34.8f | 1.6 | (2.7 (0.03)) | – | 3 | 2.3 (0.54) | 2.6 (0.42) | – | 2.45±0.2 | 3, 11 |
| HD 1835 | 14 | 25.9 | 1.0 | (3.9 (0.04)) | – | 1 | 7.8 (0.60) | 3.8 (0.28) | – | 7.8±0.2 | 2, 11, 22 |
| HD 3296 | 19 | 7.1 | 0.5 | – | – | 4 | 2.4–8 (0.3) | … | … | (6±3) | 4 |
| HD 3670i | 24 | 27.2 | 2.1 | – | – | 1 | 0.73 (0.32) | 1.44 (0.11) | – | 1.44±0.1 | 2 |
| HD 5133i | 26 | 6.8 | 0.2 | – | – | 2 | 9.9 (0.16) | 5.4 (0.14) | – | 9.9±0.5 | 2 |
| HD 5349 | 12 | 2.4 | 0.2 | – | – | 2 | 6.0 (<0.01) | 3.0 (<0.01) | (5±2) | 5, 22 | |
| HD 7570i | 28 | 6.1 | 0.3 | – | – | 3 | 5.5 (0.01) | 11 (0.01) | – | (11±2) | 2 |
| HIP 6276i | 18 | 27.3f | 0.9 | (6.0 (0.5)) | – | 1 | 5.96 (0.96) | – | – | 5.96±0.1 | 1, 11 |
| HD 10008i | 17 | 10.4 | 0.3 | – | – | 2 | 7.1 (0.27) | 3.5 (0.26) | 12.3 (0.1) | (7 or 12) | 7 |
| HD 13246i | 21 | 19.3 | 1.4 | – | – | 1 | 1.71 (0.63) | – | – | 1.71±0.1 | 1 |
| HD 14082 B | 16 | 20.8f | 0.7 | – | – | 1 | 4.09 (0.22) | 0.79 (0.18) | – | (4.1±0.3) | 8 |
| HD 15060 | 12 | 9.3 | 0.6 | – | – | 4 | 5.1 (0.04) | 8.6 (0.03) | – | (8±3) | 2, 22 |
| HD 16673 | 13 | 3208l | – | – | 2 | 5.0 (0.45) | 12.2 (0.14) | 7.9 (0.11) | (5 or 12) | 7,20 | |
| HD 17925i | 11 | 18.7f | 0.6 | – | – | 2 | 6.9 (0.52) | 4.9 (0.30) | 11.9 (0.29) | (7 or 12) | 7 |
| HD 19668i | 14 | 47.6f | 1.6 | 2.8 (<0.001) | – | 1 | 5.68 (0.59) | 2.69 (0.38) | 4.26 (0.19) | 5.7±2 | 2, 10 |
| HD 20759 | 17 | 5002l | – | – | 3 | 3–10 (0.01) | … | … | (7±3) | 4, 20, 22 | |
| HD 22484i | 11 | 2.9 | 0.2 | – | – | 1 | 4.43 (0.05) | – | – | (4.4±0.5) | la |
| HD 23356i | 11 | 4.6 | 0.1 | – | – | 2 | 6.7 (0.06) | 11.9 (0.06) | – | (12±1) | 2 |
| HD 23484i | 44 | 12.7 | 0.4 | – | – | 1 | 4.1 (0.22) | 9.0 (0.21) | 6.3 (0.15) | (9±1) | 8 |
| BD +23 551 | 19 | 41.4 | 2.3 | – | – | 3 | 2.4 (0.59) | 1.2 (0.20) | – | 2.4±0.1 | 2 |
| HD 24649 | 14 | 19.5f | 3.2 | (1.7 (0.8)) | – | 2 | 1.7 (0.62) | 1.88 (0.42) | – | 1.8±0.2 | 3, 11 |
| HD 27638 B | 16 | 26190f | – | – | 0 | … | … | … | 6, 20 | ||
| HD 28069 | 22 | 78.5 | 3.4 | – | – | 1 | 2.3 (0.78) | – | – | 2.3±0.1 | 1 |
| HD 28447 | 15 | 4.2 | 0.3 | – | – | 3 | 2.6–7 (0.01) | … | … | (5±2) | 4 |
| HD 31392 | 16 | 10.1 | 0.3 | – | – | 3 | 6.0 (0.19) | 12.6 (0.15) | – | (12±2) | 2 |
| HD 33081 | 45 | 2.9 | 0.2 | – | – | 2 | 3.5–10.5 (0.03) | … | … | (8±3) | 4 |
| SAO 150676i | 19 | 211 | 9.1 | (1.8 (0.7)) | – | 3 | 1.75 (0.8) | – | – | 1.75±0.1 | 1, 11 |
| HD 38397i | 17 | 15.8 | 0.8 | – | – | 4 | 2.27 (0.84) | – | – | 2.27±0.1 | 1 |
| HD 38949 | 14 | 14.9f | 0.6 | (3.8 (0.7)) | (9 (0.5)) | 3 | 3.8 (0.46) | 7.5 (0.38) | – | 7.5±0.3 | 2, 11, 22 |
| HD 40136i | 13 | 18.6f | 1.1 | – | – | 2 | 0.96 (0.11) | – | – | 0.96±0.1 | 1 |
| HD 43989i | 17 | 143f | 6.6 | – | – | 2 | 1.36 (0.67) | – | – | 1.36±0.1 | 1 |
| HD 48370i | 20 | 47.3f | 1.6 | – | – | 1 | 5.18 (0.87) | – | – | 5.18±0.1 | 1 |
| HD 50571 | 37 | 188f | 9.1 | – | – | 24 | 1.69 (0.12) | … | … | 1.69±0.1 | 1 |
| HD 53143 | 21 | 15.4f | 0.5 | (4.8 (0.1)) | – | 25 | 9.6 (0.6) | 4.9 (0.27) | – | 9.6±0.3 | 2, 11 |
| HD 57703 | 20 | 30.4 | 2.1 | – | – | 3 | 1.69 (0.13) | 1.9 (0.08) | – | (1.8±0.2) | 3 |
| HD 59659 | 44 | 48.4 | 3.2 | – | – | 5 | 1.64 (0.73) | – | – | 1.64±0.1 | 1 |
| HD 59967i | 28 | 14.4 | 0.5 | – | – | 3 | 5.2 (0.58) | 7.9 (0.17) | – | (6±1.5) | 3 |
| HD 72687 | 21 | 47.9f | 1.6 | 3.8 (0.05) | – | 3 | 3.8 (0.6) | 5.1 (0.27) | 1.9 (0.15) | (3.8 or 5.1) | 7, 10 |
| HD 76151i | 34 | 4.6 | 0.2 | – | – | 2 | 3.2–14 (0.15) | … | … | (8±3) | 4 |
| HD 76748 | 22 | 7.7 | 0.3 | – | – | 2 | 1.4–3 (<0.01) | – | – | … | 5, 22 |
| HD 76653 | 16 | 16.2f | 0.8 | 2.0 (<0.001) | 4 | 2.1 (0.5) | – | – | 2.1±0.2 | 1, 10 | |
| CD -49 3972 | 35 | 9.5 | 0.5 | – | – | 4 | 3.1–11.5 (0.1) | … | (7±3) | 4 | |
| HD 84075 | 16 | 92.9f | 3.9 | (2.4 (0.05)) | 5 | 2.44 (0.76) | – | – | 2.44±0.1 | 1, 11 | |
| HD 90905i | 19 | 9.7 | 0.4 | – | – | 3 | 2.55 (0.66) | – | – | 2.55±0.1 | 1 |
| HD 92945i | 14 | 27.5f | 0.9 | (3.7 (0.4)) | (7.6 (0.5)) | 2 | 3.4 (0.45) | 7.4 (0.38) | 13.5 (0.21) | (7.4 or 13.5) | 7, 11 |
| HD 93932 | 40 | 6.3 | 0.3 | – | – | 2 | 4.3 (<0.01) | 5.8 (<0.01) | – | (5±1) | 3, 22 |
| HD 101259 | 15 | 9.6 | 0.7 | – | – | 2 | 0.75–5.5 (0.02) | … | … | 5, 22 | |
| HD 102458i | 14 | 504f | 25 | 2.0 (<0.001) | – | 2 | 2.0 (0.53) | 0.85 (0.2) | – | 2.0±0.1 | 2, 10 |
| HD 102902 | 6 | 911l | – | – | 3 | 0.7 (0.13) | 1.5 (0.07) | – | 1.5±0.2 | 2, 20, 22 | |
| HD 104231i | 27 | 26.0 | 2.1 | – | – | 3 | 0.55 (0.11) | 1.04 (0.12) | – | 1.0±0.2 | 2 |
| HD 105912 | 27 | 145f | 7.4 | – | – | 1 | 0.7 (0.13) | 1.5 (0.08) | – | 1.5±0.2 | 2 |
| MML 8i | 8 | 767f | 34 | 2.4 (0.01) | – | 2 | 2.41 (0.97) | – | – | 2.4±0.1 | 1, 10, 21 |
| HD 107146i | 13 | 33.lf | 1.2 | 3.6 (0.001) | – | 0 | … | … | … | 3.6±0.3 | 6, 12, 21 |
| HD 107649i | 29 | 577 | 30 | – | – | 3 | 0.94 (0.58) | – | – | 0.94±0.1 | 1 |
| HD 108857 | 5 | 4851l | – | – | 3 | 11.4 (<0.01) | – | – | (11±2) | la, 20 | |
| HD 109832i | 59 | 804 | 45 | 1.3 (0.001) | – | 2 | 0.79 (0.30) | 1.2 (0.26) | – | 1.2±0.2 | 2, 21 |
| HD 111520i | 32 | 219f | 10.9 | – | – | 3 | 4.7 (0.27) | 1.5 (0.1) | – | (5±1) | 8 |
| HD 111631i | 17 | 7.9 | 0.2 | – | – | 0 | … | … | … | 6 | |
| HD 114082i | 26 | 75.6f | 5.1 | – | – | 1 | 1.5–4.2 (0.05) | 8 (0.02) | – | (3.5±2) | 7 |
| HD 115820i | 16 | 6282h | 368 | – | – | 3 | – | – | – | 5, 21 | |
| HD 117214 | 20 | 81.8f | 5.5 | – | – | 2 | 2.7 (0.06) | 0.55 (0.04) | – | 2.7±0.5 | 8 |
| HD 117524 | 19 | 617f | 33 | 1.8 (0.005) | – | 1 | 1.75 (0.92) | – | – | 1.75±0.1 | 1, 10, 21, 22 |
| MML 36i | 21 | 150f | 6.5 | 4.5 (0.005) | – | 1 | 4.73 (0.94) | – | – | 4.73±0.1 | 1, 10 |
| HD 118972 | 22 | 20.3 | 0.6 | – | – | 2 | 4.7 (0.6) | 9 (0.25) | – | 9±1 | 2 |
| CD -29 10609 | 40 | 37.7f | 1.3 | – | – | 0 | … | … | … | … | 6 |
| HD 122948 | 24 | 8.0 | 0.3 | – | – | 0 | … | … | … | … | 6, 22 |
| HD 125451i | 16 | 96.1 | 5.0 | – | – | 0 | … | … | … | … | 6 |
| MML 43 | 6 | 2659l | – | – | 2 | 4.2 (0.91) | – | – | 4.2±0.1 | 1, 20 | |
| HD 129590i | 6 | 11426l | – | – | 2 | 4.5 (0.7) | – | – | 4.5±0.1 | 1, 20 | |
| HD 131156 | 18 | 13.2f | 0.4 | (3.1 (0.05)) | – | 0 | … | … | … | (3.1±0.5) | 6, 13, 22 |
| HD 132950 | 34 | 8.3 | 0.3 | – | – | 0 | … | … | … | … | 6, 22 |
| HD 134910 | 22 | 49.7 | 2.3 | – | – | 1 | 3.4 (0.55) | – | – | 3.4±0.1 | 1 |
| HD 135953i | 20 | 68.0 | 3.8 | – | – | 1 | 1.9 (0.41) | 0.94 (0.10) | – | 1.9±0.1 | 2 |
| HD 138398 | 19 | 11.0 | 1.0 | – | – | 0 | … | … | … | … | 6, 22 |
| HD 139664i | 23 | 765 | 34 | – | – | 2 | 0.88 (0.23) | 1.04 (0.1) | – | 0.95±0.1 | 3, 21 |
| HD 141011 | 28 | 1712f | 82 | – | – | 2 | 0.96 (0.15) | – | – | 0.96±0.1 | 1, 21 |
| HD 141521i | 22 | 127123l | (7.9 (0.2)) | – | 1 | 7.1 (0.95) | 13.8 (0.35) | 5.0 (0.25) | 7.1±0.2 | 1, 11, 20, 22 | |
| HD 143811 | 15 | 11469l | – | – | 1 | 4.3 (0.028) | 6.4 (0.022) | 3.4 (0.019) | (5±2) | 7, 20 | |
| HD 145229 | 25 | 12.5 | 0.5 | – | – | 0 | … | … | … | … | 6, 20 |
| HD 145560 | 30 | 152 | 7.8 | – | – | 2 | 1.4 (0.54) | 0.7 (0.1) | – | 1.4±0.1 | 2 |
| HD 145972i | 19 | 1345 | 75 | (1.5 (0.8)) | – | 2 | 1.41 (0.41) | 1.54 (0.38) | – | 1.48±0.1 | 3, 11, 21 |
| HD 146181i | 20 | 73.2 | 4.4 | – | – | 1 | 1.95 (0.26) | 0.99 (0.14) | – | 1.95±0.1 | 2 |
| HD 147594 | 23 | 198 | 11 | (2.8 (0.9)) | – | 2 | 2.98 (0.8) | – | – | 2.98±0.1 | 1, 11 |
| HD 166348i | 26 | 5.2 | 0.2 | – | – | 1 | 11.6 (0.61) | 6.5 (0.17) | – | 11.6±0.1 | 2 |
| HD 170773 | 16 | 198 | 9.5 | – | – | 1 | 0.8 (0.09) | – | – | (0.8±0.2) | 1 |
| HD 180134 | 32 | 8.6 | 0.5 | – | – | 2 | 4.5 (0.005) | 12 (0.004) | 2.3 (0.003) | … | 9 |
| HD 181327i | 16 | 6.0f | 0.5 | – | – | 2 | 1.57 (0.3) | 0.75 (0.1) | – | 1.6±0.2 | 2 |
| HD 183216 | 31 | 15.7 | 0.7 | – | – | 2 | 9.5 (0.3) | 5.1 (0.2) | – | (10±2) | 2 |
| HD 187897 | 32 | 10.9 | 0.4 | – | – | 0 | … | … | … | … | 6 |
| HD 190470 | 30 | 8.9f | 0.3 | – | – | 2 | 11.3 (0.12) | 5.9 (0.08) | – | 11.3±0.5 | 2 |
| HD 191089i | 15 | 25.6 | 1.8 | – | – | 0 | … | … | … | … | 6 |
| HD 191849i | 23 | 8.7 | 0.2 | – | – | 0 | … | … | … | 6 | |
| HD 199260i | 23 | 31.9f | 1.3 | 4.1 (0.01) | – | 2 | 4.08 (0.85) | – | – | 4.08±0.1 | 1, 10 |
| HD 201219 | 29 | 14.4f | 0.5 | – | – | 0 | … | … | … | … | 6 |
| HD 202917 | 7 | 178f | 6.3 | (2.8 (0.3)) | – | 2 | 3.5 (0.8) | – | – | 3.5±0.1 | 1, 11 |
| HD 204277 | 7 | 12.8 | 0.5 | – | – | 0 | … | … | … | … | 6, 22 |
| HD 206893 | 23 | 84.6 | 4.1 | – | – | 0 | … | … | … | … | 6 |
| HD 208038 | 5 | 8.6 | 0.3 | – | – | 0 | … | … | … | … | 6, 22 |
| HD 209253i | 16 | 33.9f | 1.4 | (3.0 (0.6)) | – | 2 | 2.95 (0.60) | 1.5 (0.18) | – | 2.95±0.1 | 2, 11 |
| HD 212695i | 21 | 15.5 | 1.1 | – | – | 1 | 1.5 (0.18) | 2.8 (0.1) | – | 2.8±0.2 | 2 |
| HD 213941 | 14 | 5.2 | 0.2 | – | – | 0 | … | … | … | … | 6, 22 |
| CPD-722713i | 21 | 70.2 | 2.0 | 4.4 (<0.001) | – | 4 | 4.45 (0.95) | – | – | 4.45±0.1 | 1, 10 |
| HD 218340i | 21 | 8.7 | 0.4 | – | – | 1 | 7.7 (0.12) | – | – | 7.7±0.1 | 1 |
| HD 218511i | 41 | 7.2 | 0.2 | – | – | 3 | 8.8 (0.22) | 5.8 (0.22) | – | (9±1) | 2 |
| HD 219498i | 22 | 32.3f | 1.2 | 2.8 (0.005) | 1.5 (0.008) | 0 | … | … | … | 2.8±0.3 | 6, 12 |
| HD 219482i | 16 | 14.9f | 0.6 | 2.2 (<0.001) | – | 2 | 2.1 (0.5) | – | – | 2.1±0.1 | 1, 10 |
| HD 223340i | 13 | 24.5f | 1.2 | (6.3 (0.1)) | – | 0 | … | … | … | (6±1) | 6, 13 |
| CD –4415399 | 21 | 22.5 | 0.9 | – | – | 1 | 5.1 (<0.01) | – | – | (5.1±0.3) | la |
Notes. (a)Number of usable spectra in high–cadence RV times series. (b)rmsRV(τ 14 d) as derived from our high–cadence data.(c)Periodicities in the RV data and their false alarm probability (FAP). Non–significant periodicities are listed in brackets. (d)Periodicities in photometric TESS data and power in the GLS periodogram. All listed periods are significant. (e)Most likely stellar rotation period Prot. Uncertain guesses are listed in brackets. (f)Strong anti-correlation between BS and RV with rP ≤ –0.6 suggests RV variability is caused by rotational modulation due to starspots. (g)bf Notes regarding Prot and selection for longer-period survey: (1) Single dominant period in the photometric TESS data, (1a) Single dominant period in the photometric TESS data, but only marginally significant. (2) An approximate 2:1 ratio of two dominant photometric periods and alternating strengths and shapes in the light curve is indicative of two dominant spot groups and the longer of the two periods representing Prot. (3) Two periods close together in the photometric TESS data, we adopt the mean. (4) Multiple frequencies in the photometric TESS data, shifting between sectors, but periodogram power is limited to the given range of periods. (5) No significant periodicity in the photometric TESS data. (6) No TESS data available (yet). (7) Not clear which of the periods represents Prot. (8) The longest period most likely represents Prot. (9) Marginally significant periods, shifting between sectors, not clear indication of Prot. (10) Photometric period(s) clearly detected in RV. (11) Photometric period(s) marginally evident in RV. (12) Strong BS(RV) anti-correlation (rP ≤ −0.8) indicates that the significant RV period is caused by rotational modulation and most likley represents Prot. (13) Strong BS(RV) anti–correlation (rP ≤ −0.7) suggests that the marginally significant RV period is caused by rotational modulation and may represent Prot. (20) SB. (21) M′1yr > 80 MJup. (22) No significant debris disc signal. (h)HD 115820 turns out to be a δ Scuti varaible. The GLS periodigram of the TESS photometry shows several g-mode pulsation periods between 42 and 68 min, which explains the large RV scatter. (i)Observed with NaCo under the ISPY programme. (k)Mass detection limits for P = 10d corresponding to 3×rmsRV(τ 14d). The corresponding mass-detection limit for P = 1 yr is M′1yr = M′10d × (365/10)(1/3). (l)Spectroscopic binary (Sect. 6.4).
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