Three-Mirror Telescope. Institute of Astronomy, University of Cambridge; abgerufen im 1. Januar 1
doi.org
James G. Baker: On Improving the Effectiveness of Large Telescopes. In: IEEE Transactions on Aerospace and Electronic Systems. AES-5, Nr.2, 1969, ISSN1557-9603, S.261–272, doi:10.1109/TAES.1969.309914: „There is a possible Case 2-7. The tertiary mirror is ground and polished into the primary mirror blank to form a two-component three-mirror system.“
Dietrich Korsch: Closed Form Solution for Three-Mirror Telescopes, Corrected for Spherical Aberration, Coma, Astigmatism, and Field Curvature. In: Applied Optics. Band11, Nr.12, 1972, ISSN2155-3165, S.2986–2987, doi:10.1364/AO.11.002986.
Kyoji Nariai, Masanori Iye: Three-Mirror Anastigmat Telescope with an Unvignetted Flat Focal Plane. In: Publications of the Astronomical Society of Japan. Band57, 1. April 2005, S.391–397, doi:10.1093/pasj/57.2.391.
R. V. Willstrop: The Mersenne-Schmidt – A three-mirror survey telescope. In: Monthly Notices of the Royal Astronomical Society. Band210, 1. Oktober 1984, S.597–609, doi:10.1093/mnras/210.3.597.
Lacy G. Cook: Wide Field Of View Three-Mirror Anastigmat (TMA) Employing Spherical Secondary And Tertiary Mirrors. In: Recent Trends in Optical Systems Design: Computer Lens Design Workshop, 13-15 January 1987, Los Angeles, Calif. (= Proceedings of SPIE. Band0766). SPIE, 1987, ISBN 0-89252-801-X, S.158–162, doi:10.1117/12.940216.
Joseph M. Howard, Kong Q. Ha, Ron Shiri, J. Scott Smith, Gary Mosier, Danniella Muheim: Optical modeling activities for NASA’s James Webb Space Telescope (JWST): Part V. Operational alignment updates. In: Modeling, Systems Engineering, and Project Management for Astronomy III. Band7017. SPIE, 2008, S.295–304, doi:10.1117/12.790237.
James W. Contreras, Paul A. Lightsey: Optical design and analysis of the James Webb Space Telescope: optical telescope element. In: Conference Proceedings of the SPIE. 5524. Jahrgang, 22. Oktober 2004, doi:10.1117/12.559871 (spiedigitallibrary.org).
Bert A. Pasquale, Thomas Casey et al.: Optical design and predicted performance of the WFIRST phase-b imaging optics assembly and wide field instrument. Band10745. SPIE, 17. September 2018, S.110–120, doi:10.1117/12.2325859.}
L. G. Seppala u. a.: Optical Design for the 8.4m Large Synoptic Survey Telescope. Band205, 1. Dezember 2004, S.108.03, bibcode:2004AAS...20510803S.
U. Laux: Wide-Field-Imaging 3-Mirror-Systems with High Light Gathering Power and a Wide-Field Optical System for the „large Imaging Telescope“ (LITE). Band161, 1. Januar 1994, S.101, bibcode:1994IAUS..161..101L.
James W. Contreras, Paul A. Lightsey: Optical design and analysis of the James Webb Space Telescope: optical telescope element. In: Conference Proceedings of the SPIE. 5524. Jahrgang, 22. Oktober 2004, doi:10.1117/12.559871 (spiedigitallibrary.org).
James G. Baker: On Improving the Effectiveness of Large Telescopes. In: IEEE Transactions on Aerospace and Electronic Systems. AES-5, Nr.2, 1969, ISSN1557-9603, S.261–272, doi:10.1109/TAES.1969.309914: „There is a possible Case 2-7. The tertiary mirror is ground and polished into the primary mirror blank to form a two-component three-mirror system.“
Dietrich Korsch: Closed Form Solution for Three-Mirror Telescopes, Corrected for Spherical Aberration, Coma, Astigmatism, and Field Curvature. In: Applied Optics. Band11, Nr.12, 1972, ISSN2155-3165, S.2986–2987, doi:10.1364/AO.11.002986.