Table 2
Dependence of the disk scattering intensity and polarization on model parameters.
| Xr | Xr−1,Xr+1 |  |
 |
〈pφ〉 | |
|---|---|---|---|---|---|
| ω | 0.5 | 0.2,0.8 | 1.92 ± 0.52 (b) | 1.11 ± 0.02 | −0.54 ± 0.03 |
| ɡ | 0.5 | 0.25,0.75 | −0.64 ± 0.14 | −0.81 ± 0.10 | −0.20 ± 0.01 |
| pmax | 0.5 | 0.2,0.8 | −0.01 ± 0.01 | 1.01 ± 0.01 | 1.02 ± 0.01 |
| α | 10 | 5, 20 | 1.16 ± 0.06 | 1.12 ± 0.04 | −0.02 ± 0.01 |
| χ | 32.5 | 12.5, 57.5 | −0.65 ± 0.08 | −0.76 ± 0.03 | −0.07 ± 0.09 |
| cos i | 0.84 | 0.99, 0.61(a) | 0.12 ± 0.06 | 1.62 ± 0.03 | 1.51 ± 0.08 |
Notes. The gradients of the radiation parameters integrated intensity 
, azimuthal polarization and averaged fractional polarization 〈pφ〉 for the scattered light from transition disk with respect to the geometric parameters inclination i, angular wall height a, wall slope χ, and the dust parameters scattering albedo ω, asymmetry ɡ, and maximum scattering polarization pmax. (a)The linear relation for 
is valid to cos i = 0.61 corresponding to i = 42.5°. (b)Here the linear relation does not fit well, so we use a power law instead: 
.
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