Table 3
Data sets of Gl 486 used in this work.
| Facility (a) | Run, visit or sector | Observing dates (UT) | Filter, instrument, or channel | Nobs(used)(b) | Reference(b) | |
|---|---|---|---|---|---|---|
| Start | End | |||||
| Space photometry | ||||||
| TESS | 23 | 18 March 2020 | 16 April 2020 | T | 13 167 (13 167) | Tri21 |
| CHEOPS | 1 | 05 April 2021 | Open | 470 (429) | This work | |
| 2 | 07 April 2021 | 436 (398) | This work | |||
| 3 | 12 April 2021 | 406 (370) | This work | |||
| 4 | 15 April 2021 | 414 (372) | This work | |||
| 5 | 18 April 2021 | 396 (366) | This work | |||
| 6 | 10 June 2021 | 341 (288) | This work | |||
| 7 | 26 June 2021 | 284 (232) | This work | |||
| High-resolution spectroscopy | ||||||
| CARMENES | 1 | 13 January 2016 | 10 June 2020 | VIS | 80 (76) | Tri21 |
| 2 | 01 May 2021 | 07 May 2021 | 5 (5) | This work | ||
| MAROON-X | 1 | 20 May 2020 | 02 June 2020 | Blue, Red | 65 (65) | Tri21 |
| 2 | 16 April 2021 | 30 April 2021 | 8 (8) | This work | ||
| 3 | 25 May 2021 | 02 June 2021 | 8 (8) | This work | ||
| Interferometry | ||||||
| CHARA | 1 | 24 May 2021 | MIRC-X | 126 | This work | |
| 2 | 27 May 2021 | MIRC-X | 402 | This work | ||
| Space spectroscopy | ||||||
| Hubble (c) | 1 | 15 March 2022 | STIS G140L | 1 | This work | |
| 2 | 16 March 2022 | STIS G140M | 1 | This work | ||
| Ground photometry | ||||||
| ASAS-SN | 1 | 14 February 2012 | 26 November 2018 | V | 972 (958) | Tri21 |
| 2 | 04 December 2017 | 10 May 2020 | 1064 (1054) | Tri21 | ||
| AstroLAB | 1 | 19 May 2021 | 27 June 2021 | V | 39 (39) | This work |
| LCOGT | 1 | 22 April 2021 | 27 July 2021 | B | 440 (429) | This work |
| OSN | 1 | 17 May 2021 | 30 April 2022 | T90 V | 1729 (1729) | This work |
| SuperWASP | 1 | 5 February 2008 | 29 March 2011 | North | 182 (181) | Tri21 |
| 2 | 30 January 2013 | 15 July 2014 | South | 184 (178) | Tri21 | |
| TJO | 1 | 31 March 2021 | 24 April 2022 | LAIA R | 610 (594) | This work |
Notes. (a)TESS: Transiting Exoplanet Survey Satellite; CHEOPS: CHaracterising ExOPlanets Satellite; CARMENES: Calar Alto high-Resolution search for M dwarfs with Exoearths with Near-infrared and optical Echelle Spectrographs; MAROON-X: M-dwarf Advanced Radial velocity Observer Of Neighboring eXoplanets; CHARA: Center for High Angular Resolution Astronomy; ASAS-SN: All Sky Automated Survey for SuperNovae; LCOGT: Las Cumbres Observatory Global Telescope; OSN: Observatorio de Sierra Nevada; WASP: Wide Angle Search for Planets; TJO: Telescopi Joan Oró.(b)Number of eventually used data points in parentheses. For SuperWASP north and south, we tabulate the Nobs(used) binned per night; the actual total number of SuperWASP data amount to 51 720. (b)Data sets presented for the first time in this work or used already by Trifonov et al. (2021; Tri21). (c)Under GO 16701, there are also Hubble STIS spectra with CCD/G430L (2900-5700 Å) and NUV/G230L (1700-3200 Å).
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