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Table 4

Best-fit parameters for the cloud and magnetic spot models for each brown dwarf.

Object Retrieved γ Model γ Retrieved k0 Model k0 Δ A (%) χ2 ΔT (K) ΔA (%) χ2
2M1721+33 4.230.20+0.15Mathematical equation: $-4.23^{+0.15}_{-0.20}$ 4.110.09+0.07Mathematical equation: $-4.11^{+0.07}_{-0.09}$ 2.420.43+0.75Mathematical equation: $2.42^{+0.75}_{-0.43}$ 1.610.19+0.14Mathematical equation: $1.61^{+0.14}_{-0.19}$ 15.506.81+9.48Mathematical equation: $15.50^{+9.48}_{-6.81}$ 0.90 −200 2.890.08+0.07Mathematical equation: $2.89^{+0.07}_{-0.08}$ 0.81
2M0036+18 (epoch 1) 4.020.02+0.01Mathematical equation: $-4.02^{+0.01}_{-0.02}$ 4.000.03+0.02Mathematical equation: $-4.00^{+0.02}_{-0.03}$ 2.010.03+0.04Mathematical equation: $2.01^{+0.04}_{-0.03}$ 1.460.04+0.04Mathematical equation: $1.46^{+0.04}_{-0.04}$ 12.950.27+0.20Mathematical equation: $12.95^{+0.20}_{-0.27}$ 4.93 −200 2.950.03+0.02Mathematical equation: $2.95^{+0.02}_{-0.03}$ 3.36
2M0036+18 (epoch 2) 4.040.02+0.02Mathematical equation: $-4.04^{+0.02}_{-0.02}$ 3.870.06+0.04Mathematical equation: $-3.87^{+0.04}_{-0.06}$ 2.020.04+0.04Mathematical equation: $2.02^{+0.04}_{-0.04}$ 1.040.10+0.06Mathematical equation: $1.04^{+0.06}_{-0.10}$ 10.152.65+0.47Mathematical equation: $10.15^{+0.47}_{-2.65}$ 5.84 −200 3.250.03+0.03Mathematical equation: $3.25^{+0.03}_{-0.03}$ 4.68
2M1906+40 4.010.02+0.01Mathematical equation: $-4.01^{+0.01}_{-0.02}$ 3.030.03+0.03Mathematical equation: $-3.03^{+0.03}_{-0.03}$ 5.620.49+0.68Mathematical equation: $5.62^{+0.68}_{-0.49}$ 5.650.22+0.20Mathematical equation: $5.65^{+0.20}_{-0.22}$ 2.100.06+0.05Mathematical equation: $2.10^{+0.05}_{-0.06}$ 0.64 −300 1.460.04+0.04Mathematical equation: $1.46^{+0.04}_{-0.04}$ 0.72

Notes. k0 is the opacity of the clouds at 350nm and γ is the power-law exponent of the clouds. ∆A is the coverage fraction between the bulk atmosphere and the perturbed atmosphere (due to clouds or magnetic spots).

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