  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.
