The weak gravitational lensing (WGL) produces a shear effect on the observed galactic
ellipticity that is much smaller than the endogenous ellipticity of
the galaxy itself. Achieving such a high-level astronomical
observation requires the superior performance of telescopes. To ensure
the optical properties of telescopes to be competent in WGL
detections, it is very necessary to measure point spread function
(PSF) ellipticity of telescopes in labs. In this paper, a 2 m
off-axis telescope that would be used to detect WGL in space is
analyzed and studied. A collimator whose aperture is 2 m has
been built to measure PSF ellipticity of the telescope. The wave
aberrations of the collimator are roughly equal to those of the
telescope, so they are important systematical errors and must be
removed. However, it is difficult to precisely measure the wave
aberrations of optical systems that have large apertures and long
focal lengths. In addition, a 2 m flat mirror, which is
indispensable to measure wave aberrations of optical systems, has
significant surface errors. In this paper, a multi-objective
optimization method is proposed to eliminate the effects of wave
aberrations on PSF ellipticity measurements of the telescope. By
constructing an equivalent model, the wave aberrations from
collimators and flat mirrors can be corrected so that PSF ellipticity
measurement error is reduced to within 0.01. Measurement accuracy of
PSF ellipticity of the telescopes can be improved significantly.