Development of a wide field spherical aberration corrector for the Hobby Eberly Telescope: design, fabrication and alignment

A 4-mirror prime focus corrector is under development to provide seeing-limited images for the 10-m aperture Hobby- Eberly Telescope (HET) over a 22 arcminute wide field of view. The images created by the spherical primary mirror are aberrated with 13 arcmin diameter point spread function. The University of Arizona is developing the 4-mirror wide field corrector to compensate the aberrations from the primary mirror and present seeing limited imaged to the pickoffs for the fiber-fed spectrographs. The requirements for this system pose several challenges, including optical fabrication of the aspheric mirrors, system alignment, and operational mechanical stability. This paper presents current status of the program which covers fabrication of mirrors and structures and pretest result from the alignment of the system.

[1]  Hanshin Lee,et al.  Current status of the Hobby-Eberly Telescope wide field upgrade , 2010, Other Conferences.

[2]  James H. Burge,et al.  Alignment of four-mirror wide field corrector for the Hobby-Eberly Telescope , 2013, Optics & Photonics - Optical Engineering + Applications.

[3]  James H. Burge,et al.  Use of the Abbe sine condition to quantify alignment aberrations in optical imaging systems , 2010, International Optical Design Conference.

[4]  Darragh O'Donoghue Correction of spherical aberration in the Southern African Large Telescope (SALT) , 2000, Astronomical Telescopes and Instrumentation.

[5]  James H. Burge Certification of null correctors for primary mirrors , 1994, Optics & Photonics.

[6]  James H. Burge,et al.  Swing arm optical CMM for aspherics , 2009, Optical Engineering + Applications.

[7]  James H. Burge,et al.  Development of a wide-field spherical aberration corrector for the Hobby Eberly Telescope , 2010, Astronomical Telescopes + Instrumentation.