TOI-3493 b: A planet with a Neptune-like density transiting a bright G0-type star

Open Access

Table 5

Comparison of RV-only models.

Models	ln $Z$ $\mathcal{Z}$	$\| Δ \ln Z \|$ $\vert\Delta \ln \mathcal{Z}\vert$
Two-signal models (without activity modeling)
1cp	−227.77	7.76
1ep	−238.57	18.56
2cp	−220.02	0
1cp+1ep	−230.38	10.37
2ep	−233.95	13.94
1cp+lt	−216.75	−3.26
1cp+qt	−229.98	9.96
2cp+lt	−219.09	−0.93
2cp+qt	−219.29	−0.72
1cp+GP	−205.21	−14.80
1ep+GP	−209.53	−10.49

Notes. Here, “cp,” “ep,” lt, qt, and “GP” refer to a circular planet model, eccentric planet model, linear trend, quadratic trend, and GPs, respectively. ln $Z$ $\mathcal{Z}$ and $| Δ \ln Z |$ $|\Delta \ln Z|$ are the log-evidence and relative absolute log-evidence with respect to the fiducial model (2cp here), respectively.

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.