Abstract

Remote focusing (RF) is a technique that greatly extends the aberration-free axial scan range of an optical microscope. To maximise the diffraction limited depth range in an RF system, the magnification of the relay lenses should be such that the pupil planes of the objectives are accurately mapped on to each other. In this paper we study the tolerance of the RF system to magnification mismatch and quantify the amount of residual spherical aberration present at different focusing depths. We observe that small deviations from ideal magnification results in increased amounts of residual spherical aberration terms leading to a reduction in the diffracted limited range. For high-numerical aperture objectives, the simulation predicts a 50% decrease in the diffracted limited range for 1% magnification mismatch. The simulation has been verified against an experimental RF system with ideal and nonideal magnifications. Experimentally confirmed predictions also provide a valuable empirical method of determining when a system is close to the ideal phase matching condition, based on the sign of the spherical aberration on either side of focus.

Highlights

  • Live biological imaging requires acquisition of image volumes at high speed and high spatial resolution

  • A folded Remote focusing (RF) system was built with three different relay lens magnifications to verify the computational model

  • The first order spherical aberration term obtained from the experiments was found to be in close agreement with the simulated results

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Summary

Introduction

Live biological imaging requires acquisition of image volumes at high speed and high spatial resolution. Multifocus Microscopes[1] use distorted diffraction gratings for simultaneous imaging of multiple planes in a single camera frame acquisition These gratings are designed to compensate for spherical aberration introduced at specific depths and extends the axial (z) range of imaging using high numerical aperture (NA) objectives to a few tens of microns. Another refocusing method introduces a lenslet array into the optical path to form a Light Field Microscope[2]. Light Field Microscopes have an inherent trade-off between the extended axial range of imaging and the spatial resolution of the microscope

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