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

Open Access

Fig. 10

Integrated polarization parameters for the RingI60 model as a function of the ring radius r₀ after convolution with PSF_G (a) and PSF_AO (b). All parameters have been normalized to the intrinsic value $Σ Q_{ϕ}^{'}$ ${\rm{\Sigma }}Q_\phi ^\prime$ . In panel b the ΣQ_ϕ curve from panel a is repeated as a dotted line.

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