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  1. F. J. Low, G. Rieke, in Methods of Experimental Physics, N. Carleton, Ed. (Academic, New York, 1974), Vol. 12.
  2. C. S. L. Keay, F. J. Low, G. H. Rieke, R. B. Minton, Astrophys. J. 183, 1063 (1973).
    [CrossRef]
  3. H. M. Dyck, T. Simon, B. Zuckerman, Astrophys. J.Lett. 255, L103 (1982).
    [CrossRef]
  4. D. W. McCarthy, F. J. Low, S. G. Kleinmann, D. V. Arganbright, Astrophys. J. Lett. 259, L75 (1982).
    [CrossRef]
  5. J. Apt, R. Goody, L. Mertz, Apll. Opt. 19, 1590 (1980).
    [CrossRef]
  6. F. Sibille, A. Chelli, P. Lena, Astron. Astrophys. 79, 315 (1979).

1982 (2)

H. M. Dyck, T. Simon, B. Zuckerman, Astrophys. J.Lett. 255, L103 (1982).
[CrossRef]

D. W. McCarthy, F. J. Low, S. G. Kleinmann, D. V. Arganbright, Astrophys. J. Lett. 259, L75 (1982).
[CrossRef]

1980 (1)

J. Apt, R. Goody, L. Mertz, Apll. Opt. 19, 1590 (1980).
[CrossRef]

1979 (1)

F. Sibille, A. Chelli, P. Lena, Astron. Astrophys. 79, 315 (1979).

1973 (1)

C. S. L. Keay, F. J. Low, G. H. Rieke, R. B. Minton, Astrophys. J. 183, 1063 (1973).
[CrossRef]

Apt, J.

J. Apt, R. Goody, L. Mertz, Apll. Opt. 19, 1590 (1980).
[CrossRef]

Arganbright, D. V.

D. W. McCarthy, F. J. Low, S. G. Kleinmann, D. V. Arganbright, Astrophys. J. Lett. 259, L75 (1982).
[CrossRef]

Chelli, A.

F. Sibille, A. Chelli, P. Lena, Astron. Astrophys. 79, 315 (1979).

Dyck, H. M.

H. M. Dyck, T. Simon, B. Zuckerman, Astrophys. J.Lett. 255, L103 (1982).
[CrossRef]

Goody, R.

J. Apt, R. Goody, L. Mertz, Apll. Opt. 19, 1590 (1980).
[CrossRef]

Keay, C. S. L.

C. S. L. Keay, F. J. Low, G. H. Rieke, R. B. Minton, Astrophys. J. 183, 1063 (1973).
[CrossRef]

Kleinmann, S. G.

D. W. McCarthy, F. J. Low, S. G. Kleinmann, D. V. Arganbright, Astrophys. J. Lett. 259, L75 (1982).
[CrossRef]

Lena, P.

F. Sibille, A. Chelli, P. Lena, Astron. Astrophys. 79, 315 (1979).

Low, F. J.

D. W. McCarthy, F. J. Low, S. G. Kleinmann, D. V. Arganbright, Astrophys. J. Lett. 259, L75 (1982).
[CrossRef]

C. S. L. Keay, F. J. Low, G. H. Rieke, R. B. Minton, Astrophys. J. 183, 1063 (1973).
[CrossRef]

F. J. Low, G. Rieke, in Methods of Experimental Physics, N. Carleton, Ed. (Academic, New York, 1974), Vol. 12.

McCarthy, D. W.

D. W. McCarthy, F. J. Low, S. G. Kleinmann, D. V. Arganbright, Astrophys. J. Lett. 259, L75 (1982).
[CrossRef]

Mertz, L.

J. Apt, R. Goody, L. Mertz, Apll. Opt. 19, 1590 (1980).
[CrossRef]

Minton, R. B.

C. S. L. Keay, F. J. Low, G. H. Rieke, R. B. Minton, Astrophys. J. 183, 1063 (1973).
[CrossRef]

Rieke, G.

F. J. Low, G. Rieke, in Methods of Experimental Physics, N. Carleton, Ed. (Academic, New York, 1974), Vol. 12.

Rieke, G. H.

C. S. L. Keay, F. J. Low, G. H. Rieke, R. B. Minton, Astrophys. J. 183, 1063 (1973).
[CrossRef]

Sibille, F.

F. Sibille, A. Chelli, P. Lena, Astron. Astrophys. 79, 315 (1979).

Simon, T.

H. M. Dyck, T. Simon, B. Zuckerman, Astrophys. J.Lett. 255, L103 (1982).
[CrossRef]

Zuckerman, B.

H. M. Dyck, T. Simon, B. Zuckerman, Astrophys. J.Lett. 255, L103 (1982).
[CrossRef]

Apll. Opt. (1)

J. Apt, R. Goody, L. Mertz, Apll. Opt. 19, 1590 (1980).
[CrossRef]

Astron. Astrophys. (1)

F. Sibille, A. Chelli, P. Lena, Astron. Astrophys. 79, 315 (1979).

Astrophys. J. (1)

C. S. L. Keay, F. J. Low, G. H. Rieke, R. B. Minton, Astrophys. J. 183, 1063 (1973).
[CrossRef]

Astrophys. J. Lett. (1)

D. W. McCarthy, F. J. Low, S. G. Kleinmann, D. V. Arganbright, Astrophys. J. Lett. 259, L75 (1982).
[CrossRef]

Astrophys. J.Lett. (1)

H. M. Dyck, T. Simon, B. Zuckerman, Astrophys. J.Lett. 255, L103 (1982).
[CrossRef]

Other (1)

F. J. Low, G. Rieke, in Methods of Experimental Physics, N. Carleton, Ed. (Academic, New York, 1974), Vol. 12.

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Figures (4)

Fig. 1
Fig. 1

Visibilities observed during 25–26 Nov. 1982 for the double-star α Psc with N–S scan direction. The symbols refer to two different telescopes on Mauna Kea, Hawaii. The solid line gives the theoretically expected visibility.

Fig. 2
Fig. 2

Degraded MTFs for noise frequencies in the motion of the secondary mirror of fs, fs/3, and fs/9 (∇, ●, and ○). The maximum perturbation amplitude was assumed to be 0.76λ/D. The undisturbed MTF is given by the solid line.

Fig. 3
Fig. 3

Excess noise at spatial cutoff frequency fc = D/λ as a function of maximum perturbance amplitude for three different noise frequencies.

Fig. 4
Fig. 4

Effects of chopper noise on double-star visibility for perturbation amplitudes of 0, 0.15, 0.30, and 0.76λ/D (▾, ∇, ●, and ○). Calculations refer to a double-star separation of 1.07λ/D and a perturbation frequency of fs/9. The solid line is the theoretically expected visibility curve.

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