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Table 4

Best parameters from the SED fit using ATMO models with different data combinations.

Data Teff Mass Radius log (g) log(L/L)
(K) (MJup) (RJup)
MIRI 1555333+289$\[1555_{-333}^{+289}\]$ 75+4$\[7_{-5}^{+4}\]$ 0.710.07+0.13$\[0.71_{-0.07}^{+0.13}\]$ 4.550.41+0.21$\[4.55_{-0.41}^{+0.21}\]$ 4.550.28+0.22$\[-4.55_{-0.28}^{+0.22}\]$
MagAO+MIRI 1599288+242$\[1599_{-288}^{+242}\]$ 84+4$\[8_{-4}^{+4}\]$ 0.700.07+0.11$\[0.70_{-0.07}^{+0.11}\]$ 4.580.36+0.20$\[4.58_{-0.36}^{+0.20}\]$ 4.510.23+0.18$\[-4.51_{-0.23}^{+0.18}\]$
SPHERE+MIRI 136035+35$\[1360_{-35}^{+35}\]$ 53+5$\[5_{-3}^{+5}\]$ 0.800.02+0.03$\[0.80_{-0.02}^{+0.03}\]$ 4.310.31+0.28$\[4.31_{-0.31}^{+0.28}\]$ 4.680.02+0.03$\[-4.68_{-0.02}^{+0.03}\]$
GPI+MIRI 128919+16$\[1289_{-19}^{+16}\]$ 102+2$\[10_{-2}^{+2}\]$ 0.900.02+0.03$\[0.90_{-0.02}^{+0.03}\]$ 4.480.08+0.06$\[4.48_{-0.08}^{+0.06}\]$ 4.670.01+0.01$\[-4.67_{-0.01}^{+0.01}\]$
SPHERE+MagAO +MIRI 135934+35$\[1359_{-34}^{+35}\]$ 53+5$\[5_{-3}^{+5}\]$ 0.800.02+0.02$\[0.80_{-0.02}^{+0.02}\]$ 4.300.31+0.27$\[4.30_{-0.31}^{+0.27}\]$ 4.690.03+0.03$\[-4.69_{-0.03}^{+0.03}\]$
GPI+MagAO+MIRI 128919+16$\[1289_{-19}^{+16}\]$ 102+2$\[10_{-2}^{+2}\]$ 0.900.02+0.03$\[0.90_{-0.02}^{+0.03}\]$ 4.480.08+0.06$\[4.48_{-0.08}^{+0.06}\]$ 4.670.01+0.01$\[-4.67_{-0.01}^{+0.01}\]$

Full SED 128411+12$\[1284_{-11}^{+12}\]$ 101+1$\[10_{-1}^{+1}\]$ 0.900.02+0.02$\[0.90_{-0.02}^{+0.02}\]$ 4.470.03+0.03$\[4.47_{-0.03}^{+0.03}\]$ 4.680.01+0.01$\[-4.68_{-0.01}^{+0.01}\]$

Notes. A mass Gaussian prior of mean 10 MJup was used in all the cases. The luminosity uncertainty was rounded to 0.01.

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