Open Access
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/ν | ΔT (K) | ΔA (%) | χ2/ν |
|---|---|---|---|---|---|---|---|---|---|
| 2M1721+33 | ![]() |
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0.90 | −200 | ![]() |
0.81 |
| 2M0036+18 (epoch 1) | ![]() |
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4.93 | −200 | ![]() |
3.36 |
| 2M0036+18 (epoch 2) | ![]() |
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5.84 | −200 | ![]() |
4.68 |
| 2M1906+40 | ![]() |
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0.64 | −300 | ![]() |
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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