Open Access

Table 3

Inferred system parameters.

Parameter Units Prior Median and 68.3% CI
Star
Mean density, ρ* (g cm−3) U (5, 20) 11.7 ± 0.8
q1 TESS U (0, 1)
q2 TESS U (0, 1)
q1 ExTrA U (0, 1)
q2 ExTrA U (0, 1)
Planet b
Semi-major axis, a (au) 0.01808 ± 0.00015
Eccentricity, e
Argument of pericentre, ω (°) 240 ± 130
Inclination, ip (°)
Radius ratio, Rp /R*
Scaled semi-major axis, a/R* 11 0 ± 0 4
Impact parameter, b
Transit duration, T14 (h) 1.231 ± 0.011
T0 – 2 460 000 (BJDTDB) U (36.6907, 36.6918) 36.69124 ± 0.00010
Orbital period, P (days) U (1.522757, 1.522761) 1.5227591 ± 3 × 10−7
RV semi-amplitude, K (m s−1) U (90, 110) 98.9 ± 1.3
Radius, Rp 8.7 ± 0.4
0.77 ± 0.03
Mass, Mp (ME) 86.7 ± 1.9
(MJ) 0.273 ± 0.006
Mean density, ρp (g cm−3) 0.75 ± 0.09
Surface gravity, log gp (cgs) 3.06 ± 0.03
Equilibrium temperature, Teq (K) 694 ± 15
Insolation flux (FE) 42.5 ± 1.9
r1 U (0, 1)
r2 U (0.20, 0.24)
U (−1, 1) −0.02 ± 0.06
U (−1, 1) −0.02 ± 0.10
Candidate planet c
Semi-major axis, a (au) 0.776 ± 0.011
Eccentricity, e 0.66 ± 0.09
Argument of pericentre, ω (°) 222 ± 14
Scaled semi-major axis, a/R* 466 ± 22
T0 – 2 460 000 (BJDTDB) U (−200, 350) 92 ± 19
Orbital period, P (days) U (350, 550) 427 ± 7
RV semi-amplitude, K (m s−1) U (0, 250) 121 ± 27
Minimum mass, Mp sin i (MJ) 1.66 ± 0.26
Equilibrium temperature, Teq (K) 107±3
Insolation flux (FE) 0.0230 ± 0.0012
U (−1, 1)
U (−1, 1) −0 54 ± 0 18
RV
SPIRou jitter (m s−1) U (0.01, 80) 27 ± 5
SPIRou offset (m s−1) U (20 500, 20 800) 20662 ± 16
ESPRESSO jitter (m s−1) J (0.01, 10)
ESPRESSO offset (m s−1) U (20400, 20650) 20 571 ± 9
Photometry
Offset relative flux (Relative flux) N (0, 0.01) (b)
Jitter (ppm) J (1, 1000) (b)
Amplitude of the GP (Relative flux) J (10−6, 0.1) (b)
Timescale of the GP (days) J (0.001, 10) (b)

Notes. The table lists: prior, posterior median, and 68.3% CI. Parameters without prior are derived parameters. (a)Upper limit, 95% confidence. (b)The parameters listed for the photometry are different for each TESS sector and for each individual transit observed with each of the telescopes of ExTrA. The parameters q1 and q2 are the quadratic limb-darkening coefficients parameterised using Kipping (2013). The parameters r1 and r2 are the impact parameter and transit depth parameterised using Espinoza (2018). The planetary equilibrium temperature is computed for zero albedo and full day/night heat redistribution. IAU 2012: au = 149 597 870 700 m. , , , , , . , , . CODATA 2018: G = 6.674 30 ×10−11 m3 kg−1 s−2. U(a, b): A uniform distribution defined between a lower a and an upper b limit. J(a, b): Jeffreys (or log-uniform) distribution defined between a lower a and upper b limit. Ν(μ, σ): Normal distribution prior with mean μ, and standard deviation σ.

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