Open Access

Table 1

HD 45364, HD 202696, HD 37124, and HD 215152: planetary masses and orbital elements revised with the stability-driven approach.

Planet P [days] λ [deg] e ω [deg] m [mJup]
HD 45364 (M = 0.82 M)
HD 45364 b 30.1 ± 1.6 0.184 ± 0.008 mJup
HD 45364 c 202.6 ± 0.5 0.574 ± 0.024 mJup
 
HD 202696 (M =1.91 M)
HD 202696 b 179.4 ± 4.5 <0.0774 2.09 ± 0.15 mJup
HD 202696 c <0.0866 1.84 ± 0.19 mJup
 
HD 37124 (M = 0.83 M)
HD 37124 b 0.631 ± 0.029 mJup
HD 37124 c <0.137; <0.309(99.73%) 0.549 ± 0.051 mJup
HD 37124 d 0.623 ± 0.071 mJup
 
HD 215152 (M = 0.77 M)
HD 215152 b 5.76010(84) 169.7 ± 20.5 <0.0660 1.65 ± 0.29 m
HD 215152 c <0.0579
HD 215152 d 10.8661(28) 98.6 ± 18.4 <0.0794 2.54 ± 0.43 m
HD 215152 e 25.191(23) 71.5 ± 27.6 <0.1880 2.38 ± 0.65 m
Notation Description Notation Description
P Orbital period ω Argument of periastron
λ Mean longitude m Planetary mass
e Orbital eccentricity

Notes. The values indicated in this table are the medians of the NAFF-stable distributions, accompanied with the 68.27% confidence intervals or the upper limits on them when the distributions are one-sided. In the case of HD 45364, the new dataset of combined CORALIE + HARPS measurements generates a posterior of almost-exclusively stable solutions.

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