Resolution and calibration effects in high contrast polarimetric imaging of circumstellar scattering regions

Open Access

Fig. 4

Maps for the Ring0 models with r₀ = 12.6 mas (left), 25.2 mas (middle), and 50.4 mas (right) for the intrinsic circumstellar intensities, $I_{d}^{'} (x, y)$ $I_d^\prime (x,y)$ , and the PSF_G convolved intensity, I_d(x, y), and polarization Q_d(x, y), U_d(x, y), and Q_ϕ(x, y). Here, $Σ I_{d}^{'}$ ${\rm{\Sigma }}I_d^\prime$ is the same for all models, and ±1 for the color scale represents the same fluxes per pixel for all panels.

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