Open Access
Table 1
Mass measurements of the WASP-47 planets published in the literature.
Reference | Me/M⊕ | Mb/M⊕ | Md/M⊕ | Mc sin i/M⊕ | Method |
---|---|---|---|---|---|
Hellier et al. (2012) | – | 364 ± 16 | – | – | RV |
Neveu-VanMalle et al. (2016) | – | 360 ± 19 | – | 396 ± 70 | RV |
Dai et al. (2015) | 12.2 ± 3.7 | 370 ± 29 | 10.4 ± 8.4(†) | – | RV |
Becker et al. (2015) | <22(‡) | 15±7 | – | RV+TTV | |
Almenara et al. (2016) | 364±8 | 15.7 ± 1.1 | RV+TTV(¶) | ||
Weiss et al. (2017) | 9.1 ± 1.0 | 358 ± 12 | 13.6 ± 2.0 | 416±16 | RV+TTV |
Sinukoff et al. (2017) | 9.1 ± 1.2 | 356±12 | 12.7±2.7 | 411±18 | RV |
Vanderburg et al. (2017) | 6.8 ± 0.7 | 363 ± 7 | 13.1 ± 1.5 | 398 ± 9 | RV(§) |
Bryant & Bayliss (2022) | 6.8 ± 0.6 | 364±7 | 14.2 ± 1.3 | 399 ± 9 | RV(§) |
This work (see also Table 4) | 9.0 ± 0.5 | 374±17 | 15.5 ± 0.8 | 447 ± 20 | RV+TTV |
Notes. (†)“Detected weakly if at all” (Dai et al. 2015). (‡)Upper limit at 95% confidence (Becker et al. 2015). (§)The errors on Mb and Mc are dominated by the relative uncertainty on the stellar mass M⋆ (see Sect. 4). (¶)Photodynamical approach.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.