Table 3
Priors and results from the StarSim inversion of WASP-52 photometry.
| Parameter | Prior | Value | Ref. |
|---|---|---|---|
| Prot (days) |  |
 |
This work |
| 11.8 ± 3.3 (a) | He13 | ||
| 16.40 ± 0.04 | He13 | ||
| 15.53 ± 1.96 | Ma17 | ||
| 17.79 ± 0.05 | Lo17 | ||
| 18.06 ± 0.2 | Br19 | ||
| ΔTsp (K) |  |
575 ± 150 | This work |
| 1250–1500 | Ki16 | ||
| ~270 | Ma17 | ||
| ~950 | Br18 | ||
| 250 | Al18 | ||
| 2 230 | Br19 | ||
| Q (b) |  |
<0.31 (1σ) | This work |
| s |  |
 |
This work |
Notes. The values given correspond to the optimal solution and uncertainties are estimated from a sample of 365 equivalent solutions. Literature values for the same parameters are provided when available. (a) Obtained from spectral line broadening; (b) Q is unilaterally distributed.
References: He13: Hébrard et al. (2013); Ki16: Kirk et al. (2016); Ma17: Mancini et al. (2017); Lo17: Louden et al. (2017); Al18: Alam et al. (2018); Br18: Bruno et al. (2018); Br19: Bruno et al. (2020).
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