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Table 1

Main physical and orbital parameters of the HAT-P-11 system.

Parameter(a) Value Reference
Stellar parameters
Spectral class K4 V 1
M* (M) 0.86 ± 0.06 2
R (R) 0.76 ± 0.01 2
Teff (K) 4780 ± 50 1
[Fe/H] 0.31 ± 0.05 1
log g (log10, cgs) 4.5630.080+0.092$\[4.563_{-0.080}^{+0.092}\]$ 3
Vsys (km s−1) −63.24 ± 0.26 4
Distance (ly) 123.17 ± 0.11 4
Age (Gyr) 6.54.1+5.9$\[6.5_{-4.1}^{+5.9}\]$ 2
H 7.131 ± 0.021 5
Planetary parameters
Mp (Mj) 0.0787 ± 0.0048 This work
Rp (Rj) 0.4466 ± 0.0059 This work
Mp (M) 25.0 ± 1.5 This work
Rp (R) 4.901 ± 0.065 This work
ρp (g cm−3) 1.172 ± 0.085 This work
Teq (K) 84754+46(66342+36)$\[847_{-54}^{+46}\left(663_{-42}^{+36}\right)\]$ This work
Porb (days) 4.887802443 ± 0.000000034 6
T0 (BJDtdb) 2454 957.8132067 ± 0.0000053 6
i (deg) 89.027 ± 0.068 This work
e 0.25770.0025+0.0033$\[0.2577_{-0.0025}^{+0.0033}\]$ This work
ωp (deg) 192.03.0+2.9$\[192.0_{-3.0}^{+2.9}\]$ This work
a (au) 0.0532 ± 0.0010 This work
Kp (km s−1) 123.4 ± 9.9 This work

Notes. (a)The symbols of the parameters listed in the table have the following meanings: M – stellar mass; R – stellar radius; Teff – stellar effective temperature; [Fe/H] – stellar metallicity; log g – logarithm of stellar surface gravity; Vsys – systemic radial velocity; H – apparent magnitude in the photometric H band; Mp – planetary mass; Rp – planetary radius; ρp – planetary mean density; Teq – planetary equilibrium temperature computed at the planet-to-star distance during the secondary eclipse, assuming an inefficient (full) heat re-distribution for the derived geometrical albedo (Ag=0.4400.049+0.044)$\[\left(A_{\mathrm{g}}=0.440_{-0.049}^{+0.044}\right)\]$; Porb – orbital period; T0 – transit epoch; i – orbital inclination; e – orbital eccentricity; ωp – planetary argument of periastron; a – orbital semi-major axis; Kp -planetary radial-velocity semi-amplitude.

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