[ ] Ephemerides in Table 2 are Keplerian ephemerides used in initializing the osculating Jacobi elements of the system. They should not be used to extrapolate a linear ephemeris for the planets as these osculating values do not match the mean value of the models over the duration of the data (and on longer timescales the TTVs can have stronger non-linearities, as discussed in Teyssandier et al. 2021).
[ ] Jontof-Hutter et al. (2016) used N=2 Student's-t, not N=4.
[ ] Also see Issue #34
[ ] Equation (2) is missing \sigma_{ij}^2 in the first term on the third line, i.e. it should read: -1/2 \log(\pi\nu\sigma_{ij}^2V_1). Note that this is a term that is held constant.
[ ] In Figure 12, the three models with water/steam surface layers were computed for Fe/Mg = 0.83, while the figure caption indicates Fe/Mg = 0.75.
N=2Student's-t, notN=4.\sigma_{ij}^2in the first term on the third line, i.e. it should read:-1/2 \log(\pi\nu\sigma_{ij}^2V_1).Note that this is a term that is held constant.