Optical system for extremely large spectroscopic survey telescope
Abstract
This article presents research work on a spectroscopic survey telescope. Our idea is as follows: for such a telescope, a pure reflecting optical system is designed, which should have an aperture and a field of view (FOV) both as large as possible and excellent image quality, and then a strip lensm (lens-prism) atmospheric dispersion corrector (S-ADC) is added, only for correcting the atmospheric dispersion. Given the fund limitation and the simplicity of scaling up, some 12-m telescopes are designed as examples. Su, Korsch, and Meinel put forward the four-mirror Nasmyth systems I and II, which are used in this paper. FOVs of 1.5{\deg}, 2{\deg}, and 2.5{\deg} are selected. For all systems, the image qualities are excellent. Because the S-ADC relaxes the optical glass size restriction, this 12-m telescope with a FOV of 2.5{\deg} can be magnified in proportion to a 16-m telescope. Its etendue (from French \'etendue) and focal surface will now be the largest in the world. In such a telescope, a pure reflecting optical system can also be obtained. A subsequent coud\'e system is designed with excellent image quality.
Cite
@article{arxiv.2310.04697,
title = {Optical system for extremely large spectroscopic survey telescope},
author = {Ding-qiang Su and Hua Bai and Xiangyan Yuan and Xiangqun Cui},
journal= {arXiv preprint arXiv:2310.04697},
year = {2024}
}
Comments
SCIENCE CHINA Physics, Mechanics & Astronomy, Volume 67, Issue 7: 279511 (2024)