Fig. 9
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Observation and the deconvolutions with different PSFs. (a) Observation, (b) Deconvolution performed using the PSF estimated using a previous model Conan et al. (1998). (c) Deconvolution using the estimation with the elliptical model, (d) Deconvolution using the calibration star observed after the observation, (e) Deconvolution by Marchis et al. (2021) using a Moffat PSF profile. These images are plotted with the same intensity scale.
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