Abstract

We propose a new way of recording in which a spherical blank and a deformable mirror are used to obtain high-resolution holographic gratings. The reflection of one of the two laser recording waves upon this mirror provides the deformations necessary to image correction to as much as seventh-order aberrations inclusively.

© 1998 Optical Society of America

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References

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  1. M. Duban, “Holographic aspheric gratings printed with aberrant wave,” Appl. Opt. 26, 4263–4273 (1987).
    [CrossRef] [PubMed]
  2. M. Duban, “Comparison of grating designs for the Lyman far-ultraviolet spectroscopic explorer spectrograph,” Appl. Opt. 32, 4253–4264 (1993).
    [CrossRef] [PubMed]
  3. G. R. Lemaitre, M. Wang, “Active mirrors warped using Zernike polynomials,” Astron. Astrophys. Suppl. Ser. 114, 373–378 (1995).
  4. G. R. Lemaitre, “Active procedure for making Schmidt corrector plates,” Appl. Opt. 11, 1630–1636 (1972).
    [CrossRef]
  5. G. R. Lemaitre, “Various aspect of active optics,” in Active Telescope Active Systems, F. J. Roddier, ed., Proc. SPIE1114, 328–341 (1989).
    [CrossRef]
  6. J. Green, “The Cosmic Origins Spectrograph,” Report P97-752, 1, 1997 (Center for Astrophysics & Space Astronomy, Colorado University, Boulder, Colo., 1997).

1995 (1)

G. R. Lemaitre, M. Wang, “Active mirrors warped using Zernike polynomials,” Astron. Astrophys. Suppl. Ser. 114, 373–378 (1995).

1993 (1)

1987 (1)

1972 (1)

Duban, M.

Green, J.

J. Green, “The Cosmic Origins Spectrograph,” Report P97-752, 1, 1997 (Center for Astrophysics & Space Astronomy, Colorado University, Boulder, Colo., 1997).

Lemaitre, G. R.

G. R. Lemaitre, M. Wang, “Active mirrors warped using Zernike polynomials,” Astron. Astrophys. Suppl. Ser. 114, 373–378 (1995).

G. R. Lemaitre, “Active procedure for making Schmidt corrector plates,” Appl. Opt. 11, 1630–1636 (1972).
[CrossRef]

G. R. Lemaitre, “Various aspect of active optics,” in Active Telescope Active Systems, F. J. Roddier, ed., Proc. SPIE1114, 328–341 (1989).
[CrossRef]

Wang, M.

G. R. Lemaitre, M. Wang, “Active mirrors warped using Zernike polynomials,” Astron. Astrophys. Suppl. Ser. 114, 373–378 (1995).

Appl. Opt. (3)

Astron. Astrophys. Suppl. Ser. (1)

G. R. Lemaitre, M. Wang, “Active mirrors warped using Zernike polynomials,” Astron. Astrophys. Suppl. Ser. 114, 373–378 (1995).

Other (2)

G. R. Lemaitre, “Various aspect of active optics,” in Active Telescope Active Systems, F. J. Roddier, ed., Proc. SPIE1114, 328–341 (1989).
[CrossRef]

J. Green, “The Cosmic Origins Spectrograph,” Report P97-752, 1, 1997 (Center for Astrophysics & Space Astronomy, Colorado University, Boulder, Colo., 1997).

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Equations (3)

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z =   A n , m r n   cos   m θ ,
z = 5.623 × 10 - 8 r 3   cos   θ + 4.186 × 10 - 11 r 4 - 5.623 × 10 - 8 r 3   cos   3 θ - 4.186 × 10 - 11 r 4   cos   4 θ ,
z = 5.623 × 10 - 8 r 3   cos   θ + 4.280 × 10 - 11 r 4 - 5.623 × 10 - 8 r 3   cos   3 θ - 5.413 × 10 - 11 r 4   cos   2 θ + 1.135 × 10 - 11 r 4 cos   4 θ .

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