Open Access

Table 3

Properties of the TOI-178 b, c, and d planets based on our global transit analysis (see Sect. 4.1).

Parameter (unit) Leleu et al. (2021a) This work
TOI-178
Transit depth, dF (ppm)
Transit impact parameter, b (R)
Orbital period, P (d) 1.914558 ± 0.000018
Mid-transit time, T0 (BJDTDB − 2 450 000)
Transit duration, W (h)
Orbital inclination, ip (deg)
Orbital semi-major axis, ap (au) 0.02607 ± 0.00078
Scale parameter, ap/R
Radius, Rp (R) (6.3%) 1.142 ± 0.058 (5.1%)
Stellar irradiation, Sp (S) 198 ± 14

TOI-178 c
Transit depth, dF (ppm)
Transit impact parameter, b (R) 0.24 ± 0.14
Orbital period, P (d) 3.238449 ± 0.000011
Mid-transit time, T0 (BJDTDB − 2 450 000) 8 926.0680 ± 0.0011
Transit duration, W (h)
Orbital inclination, ip (deg)
Orbital semi-major axis, ap (au) 0.0370 ± 0.0011
Scale parameter, ap/R
Radius, Rp (R) (6.8%) (3.1%)
Stellar irradiation, Sp (S) 98.3 ± 7.2
Orbital eccentricity (TTVs), ep

TOI-178 d
Transit depth, dF (ppm)
Transit impact parameter, b (R)
Orbital period, P (d) 6.557700 ± 0.000016 6.557721 ± 0.000013
Mid-transit time, T0 (BJDTDB − 2 450 000) 8 760.26373 ± 0.00074
Transit duration, W (h)
Orbital inclination, ip (deg)
Orbital semi-major axis, ap (au) 0.0592 ± 0.0018
Scale parameter, ap/R
Radius, Rp (R) (3.0%) (2.4%)
Stellar irradiation, Sp (S) 38.4 ± 2.8
Orbital eccentricity (TTVs), ep

Notes. For planets c and d, we also give the eccentricities derived from our TTV analysis (see Sect. 5). For each parameter, we indicate the median of the posterior distribution, along with the 1σ credible intervals. For the planetary radii, we also give the relative uncertainties in brackets.

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.