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Table 2

Summary of literature and derived planet properties for HR 8799 c.

Planet Ref. Clouds M (MJup) log g (cgs) Teff (K) R (RJup) [M/H] C/O log Lbol/L
c C11 Thick 7–17.5 4–4.5 1000–1200 0 −4.7 ± 0.1
G11 Slab 1.1 3.5 1200 0.97 −4.7 ± 0.1
M11 Power law 3–11 4.0–4.3 950–1025 −4.7 ± 0.1
M12 AM01 8–11 4.1 ± 0.1 950 ± 60 1.32–1.39 0 −4.90 ± 0.1
K13 3–7 3.5–4.0 1100 ± 100 1–1.5 0.65 ± 0.1
B16 ER4 3.8–3.9 1200 1.0 0.5
L17 Mie 4.5 ± 0.1 960 ± 20(a) 1.25 ± 0.02 0.55 ± 0.01
G18 Various 3.5–4.0 1100–1350 0.7–1.2 −4.58 to −4.82
W20 Deck 3.970.03+0.03$\[3.97_{-0.03}^{+0.03}\]$ 10545+7$\[1054_{-5}^{+7}\]$ 1.47 ± 0.02 0.580.06+0.06$\[0.58_{-0.06}^{+0.06}\]$ −4.59 ± 0.004
W20(b) Deck 3.950.12+0.04$\[3.95_{-0.12}^{+0.04}\]$ 1102 ± 2 1.20 0.390.06+0.06$\[0.39_{-0.06}^{+0.06}\]$ −4.69 ± 0.0002
W21(c) BT-Settl 5.40.2+0.1$\[5.4_{-0.2}^{+0.1}\]$ 1474.436.3+24.4$\[1474.4_{-36.3}^{+24.4}\]$
R21(d) Slab 3.630.02+0.03$\[3.63_{-0.02}^{+0.03}\]$ 120014+*$\[1200_{-14}^{+*}\]$ 0 0.5620.005+0.004$\[0.562_{-0.005}^{+0.004}\]$
W23 AM01 4.170.47+0.41$\[4.17_{-0.47}^{+0.41}\]$ 142172+92(e)$\[1421_{-72}^{+92(e)}\]$ 1.010.08+0.09$\[1.01_{-0.08}^{+0.09}\]$ 0.510.43+0.40(f)$\[0.51_{-0.43}^{+0.40}(f)\]$ 0.670.15+0.12$\[0.67_{-0.15}^{+0.12}\]$

Best AB AM01 8.50.4+0.4$\[8.5_{-0.4}^{+0.4}\]$ 4.260.03+0.02$\[4.26_{-0.03}^{+0.02}\]$ 115812+11$\[1158_{-12}^{+11}\]$ 1.100.01+0.01$\[1.10_{-0.01}^{+0.01}\]$ 1.270.06+0.06$\[1.27_{-0.06}^{+0.06}\]$ 0.660.01+0.01$\[0.66_{-0.01}^{+0.01}\]$ 4.710.02+0.02$\[-4.71_{-0.02}^{+0.02}\]$
BMA AB AM01 8.50.5+0.4$\[8.5_{-0.5}^{+0.4} \]$ 4.260.03+0.02$\[4.26_{-0.03}^{+0.02} \]$ 115912+11$\[1159_{-12}^{+11} \]$ 1.100.01+0.01$\[1.10_{-0.01}^{+0.01} \]$ 1.270.06+0.05$\[1.27_{-0.06}^{+0.05} \]$ 0.660.01+0.01$\[0.66_{-0.01}^{+0.01} \]$ 4.710.02+0.02$\[-4.71_{-0.02}^{+0.02}\]$
AB AM01 8.60.4+0.4$\[8.6_{-0.4}^{+0.4}\]$ 4.250.14+0.04$\[4.25_{-0.14}^{+0.04}\]$ 115976+24$\[1159_{-76}^{+24}\]$ 1.100.03+0.23$\[1.10_{-0.03}^{+0.23}\]$ 1.20.1+0.1$\[1.2_{-0.1}^{+0.1}\]$ 0.630.02+0.05$\[0.63_{-0.02}^{+0.05}\]$ 4.700.03+0.03$\[-4.70_{-0.03}^{+0.03}\]$
Grids Various 1.24–10.3 3.5–4.5 1100–1200 0.8–1.31 > 1.0 0.3–0.8 −4.65 to −4.72

Notes. (a) Only Tint, a model parameter, is reported. (b) W20 compared using strong and weak radius priors to enforce physicality. (c) W21 used high resolution spectroscopy, and did not infer masses or radii, using masses of 7.2 ± 0.7 MJup for the inner three planets and 5.8 ± 0.5 MJup for HR 8799 b. A radius of 1.2 ± 0.1 RJup was used for all planets. (d) R21 uncertainties were limited by the coarseness and boundaries of their model grid.(e) W23 report the temperature at 3.3 bar rather than the effective temperature.(f) The metallicity of W23 was found by averaging the retrieved C/H and O/H ratios.

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