Table 1
Log of RM observations.
| Target | Instrument | Night | Program (PI) | S/N | Ndata | texp (s) | RM analysis |
|---|---|---|---|---|---|---|---|
| HAT-P-3 b | HARPS-N | 30 January 2020 | OPT19B_8 (V. Bourrier) | 28.3 | 24 | 900 | − |
| HAT-P-11 b | HARPS-N | 13 September 2015 | OPT15B_19 (D. Ehrenreich) | 45.3 | 87 | 300 | − |
| HARPS-N | 01 November 2015 | OPT15B_19 (D. Ehrenreich) | 40.4 | 52 | 300 | − | |
| CARMENES | 07 August 2017 | OPT17B_026/51 (R. Allart) | 92.7 | 60 | 400 | − | |
| CARMENES | 12 August 2017 | OPT17B_026/51 (R. Allart) | 102.6 | 55 | 400 | − | |
| HAT-P-33 b | HARPS-N | 04 December 2019 | OPT19B_8 (V. Bourrier) | 20.4 | 56 | 400 | − |
| HAT-P-49 b | HARPS-N | 30 July 2020 | OPT20A_8 (V. Bourrier) | 23.1 | 126 | 180 (†) | − |
| HD 89345 b | HARPS-N | 02 February 2020 | OPT19B_8 (V. Bourrier) | 23.0 | 140 | 180 | − |
| HD 106315 c | HARPS | 09 March 2017 | 098.C-0304 (D. Ehrenreich) | 62.1 | 74 | 350 | Zhou et al. (2018) |
| HARPS | 30 March 2017 | 098.C-0304 (D. Ehrenreich) | 65.0 | 47 | 600 | Zhou et al. (2018) | |
| HARPS | 23 March 2018 | 0100.C-0750 (D. Ehrenreich) | 82.7 | 47 | 600 | − | |
| K2-105 b | HARPS-N | 18 January 2020 | OPT19B_8 (V. Bourrier) | 19.4 | 35 | 600 | − |
| Kepler-25 c | HARPS-N | 14 June 2019 | OPT19A_8 (V. Bourrier) | 36.5 | 47 | 500 | − |
| Kepler-63 b | HARPS-N | 13 May 2020 | OPT20A_8 (V. Bourrier) | 14.9 | 13 | 900 | − |
| Kepler-68 b | HARPS-N | 03 August 2019 | OPT19A_8 (V. Bourrier) | 30.7 | 72 | 300 | − |
| WASP-47 d | HARPS-N | 30 July 2021 | OPT20A_8 (V. Bourrier) | 20.2 | 19 | 900 | − |
| WASP-107 b | HARPS | 06 April 2014 | 093.C-0474 (A. H. M. J. Triaud) | 13.8 | 25 | 750 (‡) | − |
| 01 February 2018 | 0100.C-0750 (D. Ehrenreich) | 26.8 | 24 | 800 | − | ||
| 13 March 2018 | 0100.C-0750 (D. Ehrenreich) | 26.2 | 34 | 800 | − | ||
| CARMENES | 24 February 2018 | DDT.S18.188 (R. Allart) | 37.7 | 19 | 950 | − | |
| WASP-156b | CARMENES | 28 September 2019 | OPT19B_032/53 (R. Allart) | 52.6 | 17 | 1200 | − |
| 25 October 2019 | OPT19B_032/52 (R. Allart) | 58.7 | 19 | 1200 | − | ||
| 10 December 2019 | OPT19B_032/52 (R. Allart) | 49.8 | 20 | 890 | − | ||
| WASP-166 b | HARPS | 14 January 2017 | 098.C-0304 (D. Ehrenreich) | 52.6 | 71 | 300 | Hellier et al. (2019) |
| 04 March 2017 | 098.C-0304 (D. Ehrenreich) | 58.7 | 52 | 300 | Hellier et al. (2019) | ||
| 15 March 2017 | 098.C-0304 (D. Ehrenreich) | 49.8 | 65 | 350 | Hellier et al. (2019) |
Notes. The signal-to-noise ratio (S/N), number of data points Ndata, and exposure time texp relate to the exposures kept in our analysis. Time-averaged S/N are given at 550 nm for HARPS and HARPS-N, and at 785 nm for CARMENES. For each planet we indicate whether datasets were already published for RM purposes.(†) The first seven exposures were obtained with texp = 360 s. (‡)The last four exposures were obtained with texp = 900 s. (‡†)The first two exposures were obtained with texp = 400 s.
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