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References

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  1. H. M. Brandt, Glastech. Ber. 16, 123 (1938).
  2. J. E. Kupperian, A. Bogges, J. E. Milligan, Astrophys. J. 128, 453 (1958).
    [CrossRef]

1958

J. E. Kupperian, A. Bogges, J. E. Milligan, Astrophys. J. 128, 453 (1958).
[CrossRef]

1938

H. M. Brandt, Glastech. Ber. 16, 123 (1938).

Bogges, A.

J. E. Kupperian, A. Bogges, J. E. Milligan, Astrophys. J. 128, 453 (1958).
[CrossRef]

Brandt, H. M.

H. M. Brandt, Glastech. Ber. 16, 123 (1938).

Kupperian, J. E.

J. E. Kupperian, A. Bogges, J. E. Milligan, Astrophys. J. 128, 453 (1958).
[CrossRef]

Milligan, J. E.

J. E. Kupperian, A. Bogges, J. E. Milligan, Astrophys. J. 128, 453 (1958).
[CrossRef]

Astrophys. J.

J. E. Kupperian, A. Bogges, J. E. Milligan, Astrophys. J. 128, 453 (1958).
[CrossRef]

Glastech. Ber.

H. M. Brandt, Glastech. Ber. 16, 123 (1938).

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Figures (1)

Fig. 1
Fig. 1

Fields of view of the photometer for seven different wavelengths. On the ordinate are plotted the normalized anode currents of the photometer, when being turned relative to the direction of the incident light beam. The turning angle is plotted on the abscissa. The measurements were made for six different wavelengths at 2000 Å, 2250 Å, 2500 Å, 3100 Å, 3500 Å, and 4000 Å. The dotted field of view for 1900 Å is calculated. The geometrical field of view, as determined by the diaphragm in the photometer extends from −1.4 to +1.4°. Within ±2° on the abscissa the fields of view for all wavelengths are almost equal and so only one is plotted.

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