# Design of an Afocal Telescope System Integrated with Digital Imaging for Enhanced Optical Performance

## TL;DR

This paper describes a new afocal telescope system with digital imaging that improves optical performance by reducing aberrations and ensuring efficient energy transfer.

## Contribution

The novel integration of an afocal telescope with a digital imaging subsystem achieves high-resolution imaging with minimal aberrations.

## Key findings

- The system achieves an overall magnification of 16× with near-diffraction-limited quality (RMS wavefront error of 0.0474λ and Strehl ratio of 0.915).
- The MTF reaches 0.42 at 80 lp/mm with distortion below 4.87%.
- Chromatic performance is well controlled with lateral color deviations under 1.52 µm across tested wavelengths.

## Abstract

This study presents the design and optimization of a digital-imaging afocal telescope system that integrates an afocal telescope architecture with an imaging optical subsystem. The proposed system employs a combination of spherical and aspherical optical elements to enhance imaging flexibility, reduce aberrations, and ensure effective system coupling. Proper pupil matching is achieved by aligning the exit pupil of the afocal telescope with the entrance pupil of the imaging system, ensuring minimal vignetting and optimal energy transfer. Circular apertures and lens elements are used throughout the system to simplify alignment and minimize pupil-matching errors. The complete system comprises three imaging optical subsystems and a digital camera module, each independently optimized to ensure balanced optical performance. The design achieves an overall magnification of 16×, with near-diffraction-limited quality confirmed by an RMS wavefront error of 0.0474λ and a Strehl ratio of 0.915. The modulation transfer function (MTF) reaches 0.42 at 80 lp/mm, while the distortion remains below 4.87%. Chromatic performance is well controlled, with maximum lateral color deviations of 1.007 µm (short-to-long wavelength) and 1.52 µm (short-to-reference wavelength), evaluated at 656 nm, 587 nm, and 486 nm. The results demonstrate that the proposed digital-imaging afocal telescope system provides high-resolution, low-aberration imaging suitable for precision optical applications.