[1] SEBRING T A, DUNHANM E, MILLIS R, et al. The discovery channel telescope: a wide field telescope in northern arizona［C］. SPIE, 2004, 5489: 658666.

[2] KREMER R M, DEBOO B J, SASIAN J M, et al. Null corrector design for white light scatterplate interferometry on a large conic surface［C］. SPIE, 2001, 4442: 2633.

[3] QUAN Guiqin, AN Yuying, LI Qingguo, et al. Test of large aperture parabola mirror by laser interferometric［J］. Acta Photonica Sinica, 2008, 37(10): 20352038.

[4] MING Ming, WANG Jianli, MA Peili. A new method for testing the whole lens group［J］. Acta Photonica Sinica, 2011, 40(3): 419423.

[5] MING Ming, YANG Fei, CHEN Baogang, et al. The mistake during the process of testing aspheric mirror using compensator［J］. OptoElectronic Engineering, 2010, 37(10): 116121.

[6] CHEN Wei. Interferogram processing method of optical surface［J］. Acta Photonica Sinica, 2011, 40(8): 11911195.

[7] LIU Juanjuan, GUO Banghui, WU Hongshen, et al. Design of 300~1 100 nm boardwaveband optical system［J］. Acta Photonica Sinica, 2010, 39(10): 17661769.

[8] MALACARA Z, MALACARADOBLADO D, MALACARAHERNANDEZ D, et al. Astigmatic optical surface,characteristics,testing,and differences between them［J］. Optical Engineering, 2007, 46(12): 12300119.

[9] SEONG K, GREIVENKAMP J E. Surface figure measurement based on the transmitted wavefront with reverse raytracing［J］. Optical Engineering, 2008, 47(4): 043602112.

[10] KUMLER J J, CALDWELL J B. Measuring surface slope error on precision aspheres［C］. SPIE, 2007, 6671: u01u09.