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References

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  1. H. Furumoto, H. Ceccon, Appl. Phys. Lett. 13, 335 (1968).
    [CrossRef]
  2. N. C. Peterson, M. J. Kurylo, W. Braun, A. M. Bass, R. A. Keller, J. Opt. Soc. Am. 61, 746 (1971).
    [CrossRef]
  3. R. A. Keller, E. F. Zalewski, N. C. Peterson, J. Opt. Soc. Am. 61 (Dec.1971).
    [CrossRef]
  4. A. M. Bass, K. G. Kessler, J. Opt. Soc. Am. 49, 1223 (1959).
    [CrossRef]
  5. C. F. Dewey, L. O. Hocker, Appl. Phys. Lett. 18, 58 (1971).
    [CrossRef]

1971

N. C. Peterson, M. J. Kurylo, W. Braun, A. M. Bass, R. A. Keller, J. Opt. Soc. Am. 61, 746 (1971).
[CrossRef]

R. A. Keller, E. F. Zalewski, N. C. Peterson, J. Opt. Soc. Am. 61 (Dec.1971).
[CrossRef]

C. F. Dewey, L. O. Hocker, Appl. Phys. Lett. 18, 58 (1971).
[CrossRef]

1968

H. Furumoto, H. Ceccon, Appl. Phys. Lett. 13, 335 (1968).
[CrossRef]

1959

Bass, A. M.

Braun, W.

Ceccon, H.

H. Furumoto, H. Ceccon, Appl. Phys. Lett. 13, 335 (1968).
[CrossRef]

Dewey, C. F.

C. F. Dewey, L. O. Hocker, Appl. Phys. Lett. 18, 58 (1971).
[CrossRef]

Furumoto, H.

H. Furumoto, H. Ceccon, Appl. Phys. Lett. 13, 335 (1968).
[CrossRef]

Hocker, L. O.

C. F. Dewey, L. O. Hocker, Appl. Phys. Lett. 18, 58 (1971).
[CrossRef]

Keller, R. A.

N. C. Peterson, M. J. Kurylo, W. Braun, A. M. Bass, R. A. Keller, J. Opt. Soc. Am. 61, 746 (1971).
[CrossRef]

R. A. Keller, E. F. Zalewski, N. C. Peterson, J. Opt. Soc. Am. 61 (Dec.1971).
[CrossRef]

Kessler, K. G.

Kurylo, M. J.

Peterson, N. C.

N. C. Peterson, M. J. Kurylo, W. Braun, A. M. Bass, R. A. Keller, J. Opt. Soc. Am. 61, 746 (1971).
[CrossRef]

R. A. Keller, E. F. Zalewski, N. C. Peterson, J. Opt. Soc. Am. 61 (Dec.1971).
[CrossRef]

Zalewski, E. F.

R. A. Keller, E. F. Zalewski, N. C. Peterson, J. Opt. Soc. Am. 61 (Dec.1971).
[CrossRef]

Appl. Phys. Lett.

H. Furumoto, H. Ceccon, Appl. Phys. Lett. 13, 335 (1968).
[CrossRef]

C. F. Dewey, L. O. Hocker, Appl. Phys. Lett. 18, 58 (1971).
[CrossRef]

J. Opt. Soc. Am.

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Figures (4)

Fig. 1
Fig. 1

G1, grating (1800 lines/mm), first order efficiency ~90%; M1, 90R, 10T, mirror (planar); F, flashlamp; D, dye cell; M2, 60R, 40T, mirror (planar, 30′ wedge); G2, grating (2160 lines/mm), first order efficiency ~60%; L, He–Ne alignment laser; S, spectrograph.

Fig. 2
Fig. 2

Tuning the dye laser: (a) Grating G2 blocked and grating G1 tuned; (b) grating G1 blocked and grating G2 tuned. The mercury calibration lines are labeled in b.

Fig. 3
Fig. 3

Top: Grating G2 set at red end of tuning range and grating G1 tuned; Bottom: grating G2 set at blue end of tuning range and grating G1 tuned. The mercury calibration lines are labeled in Fig. 2.

Fig. 4
Fig. 4

Tuning in middle range of grating G2 by decreasing the optical feedback through mirror M2 with a polarizer. 1, 8, Hg calibration spectra; 2, no polarizer in front of grating; 3–7 optical feedback decreased by rotating polarizer through 90°.

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