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Table 2

RV observations summary.

System Instrument Mode Mask N RVs (used) Start (UT)/end (UT) RMS (m/s) S/N σRV (m/s) EXP (s)
TOI-1836 SOPHIE HR G2 89 (85) July 2020/October 2023 13.6 48 6.0 1073
TOI-2295 SOPHIE HR G2 46 (44) October 2020/October 2023 81.6 41 2.9 722
TOI-2537 SOPHIE HE G2 48 (46) August 2019/ February 2024 118.3 23 19.7 1643
TOI-2537 HARPS HR G2 22 (21) Janurary 2021/ November 2023 94.1 20 14.9 1800
TOI-2537 FEROS HR G2 19 (19) December 2020/ March 2022 116.8 50 11.6 1500
TOI-4081 SOPHIE HR G2 43 (38) August 2021/ October 2023 182.2 28 32.5 1500
TOI-4168 SOPHIE HR G2 15 (15) December 2021/ February 2024 23029.7 19 8.6 1646
TOI-5076 SOPHIE HR K5 45 (39) March 2022/February 2024 11.0 33 4.0 1118
TOI-5110 SOPHIE HR G2 23 (23) February 2022/ October 2023 133.5 29 6.5 1318

Notes. ‘HR’ and ‘HE’ represent the high-resolution and high-efficiency observation modes of SOPHIE. The observing start/end column does not indicate continuous observation. ‘N RVs’ represents the total number of RV observations, with the number of observations used in this study shown in parentheses. σRV represents RV error bars. Additionally, ‘RMS’ indicates the root mean square of final RVs, calculated after processing mentioned in Sects. 2.2, 2.3, and 2.4. The S/N of SOPHIE and HARPS are measured per pixel at 550 nm, whereas the S/N of FEROS is measured per resolution element. The columns for S/N, exposure time (‘EXP’), and σRV represent the average values for each star.

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