Abstract

Three-dimensional images of confocal laser scanning microscopy suffer from a depth-variant blur, due to refractive index mismatch between the different mediums composing the system as well as the specimen, leading to optical aberrations. Our goal is to develop an image restoration method for 3D confocal microscopy taking into account the blur variation with depth. The difficulty is that optical aberrations depend on the refractive index of the biological specimen. The depth-variant blur function or the Point Spread Function (PSF) is thus different for each observation. A blind or semi-blind restoration method needs to be developed for this system. For that purpose, we use a previously developed algorithm for the joint estimation of the specimen function (original image) and the 3D PSF, the continuously depth-variant PSF is approximated by a convex combination of a set of space-invariant PSFs taken at different depths. We propose to add to that algorithm a pupil-phase constraint for the PSF estimation, given by the the optical instrument geometry. We thus define a blind estimation algorithm by minimizing a regularized criterion in which we integrate the Gerchberg-Saxton algorithm allowing to include these physical constraints. We show the efficiency of this method relying on some numerical tests.

Highlights

  • Confocal laser scanning microscopy allows to observe in three dimensions (3D) biological living specimens, at a resolution of few hundred nanometers

  • We considered an approximation of the 3D DV Point Spread Function (PSF) by a convex combination of a set of space-invariant (SI) PSFs taken at different depths [1]

  • We propose to add an additional constraint on the PSF coming from modeling the optical instruments

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Summary

Introduction

Confocal laser scanning microscopy allows to observe in three dimensions (3D) biological living specimens, at a resolution of few hundred nanometers. We propose to incorporate these constraints in the joint image and PSF estimation algorithm presented in [1]. The PSFs are initialized from the theoretical PSF model that we present by setting approximately its physical parameters (namely the refractive index of the immersion medium and the sample). The term Pd (kx, ky, z) models the defocus of the optical instruments and is assumed to be known since it is given by the system physical parameters [5]. The support C of the aberration term is a disk of radius given by the numerical aperture (N A) of the microscope: This model allows us to impose additional constraints on the PSF (shape and support)

Blind restoration with pupil phase constraints
Numerical experiments
Full Text
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