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  1. G. R. Harrison, Phys. Rev. 45, 760 (1934).
  2. G. R. Harrison, J. Opt. Soc. Am. 19, 301 (1929).
  3. H. Kayser, Handbuch der Spektroskopie, Vol. I, p. 644. Kayser says this device saved over half the time previously required for plate measurement. See also O. Lohse, Zeits. f. Inst. 30, 169 (1910).
  4. H. E. Edgerton and K. J. Germeshatusen, Rev. Sci. Inst. 3, 535 (1932).
  5. L. G. Hoxton, Phys. Rev. 10, 90 (1917); J. Opt. Soc. Am. and Rev. Sci. Inst. 18, 442 (1929); Hoxton and D. W. Mann, Bull. Am. Phys. Soc. 10, 8 (1935). S. Grassmann, Physik. Zeits. 32, 148 (1931). H. Conrad-Billroth, Zeits. f. Inst. 54, 301 (1934).
  6. J. W. Horton, J. Frank. Inst. 216, 749 (1933). I am greatly indebted to Dr. Horton for calling the possibilities of his amplifier to my attention in this connection, and for much valuable advice regarding the electrical circuits used in the line-setting device.
  7. F. W. Sears, J. Opt. Soc. Am. 25, 162 (1935).
  8. A. C. Hardy, J. Opt. Soc. Am. 24, 162 (1934).

Edgerton, H. E.

H. E. Edgerton and K. J. Germeshatusen, Rev. Sci. Inst. 3, 535 (1932).

Germeshatusen, K. J.

H. E. Edgerton and K. J. Germeshatusen, Rev. Sci. Inst. 3, 535 (1932).

Hardy, A. C.

A. C. Hardy, J. Opt. Soc. Am. 24, 162 (1934).

Harrison, G. R.

G. R. Harrison, Phys. Rev. 45, 760 (1934).

G. R. Harrison, J. Opt. Soc. Am. 19, 301 (1929).

Horton, J. W.

J. W. Horton, J. Frank. Inst. 216, 749 (1933). I am greatly indebted to Dr. Horton for calling the possibilities of his amplifier to my attention in this connection, and for much valuable advice regarding the electrical circuits used in the line-setting device.

Hoxton, L. G.

L. G. Hoxton, Phys. Rev. 10, 90 (1917); J. Opt. Soc. Am. and Rev. Sci. Inst. 18, 442 (1929); Hoxton and D. W. Mann, Bull. Am. Phys. Soc. 10, 8 (1935). S. Grassmann, Physik. Zeits. 32, 148 (1931). H. Conrad-Billroth, Zeits. f. Inst. 54, 301 (1934).

Kayser, H.

H. Kayser, Handbuch der Spektroskopie, Vol. I, p. 644. Kayser says this device saved over half the time previously required for plate measurement. See also O. Lohse, Zeits. f. Inst. 30, 169 (1910).

Sears, F. W.

F. W. Sears, J. Opt. Soc. Am. 25, 162 (1935).

Other (8)

G. R. Harrison, Phys. Rev. 45, 760 (1934).

G. R. Harrison, J. Opt. Soc. Am. 19, 301 (1929).

H. Kayser, Handbuch der Spektroskopie, Vol. I, p. 644. Kayser says this device saved over half the time previously required for plate measurement. See also O. Lohse, Zeits. f. Inst. 30, 169 (1910).

H. E. Edgerton and K. J. Germeshatusen, Rev. Sci. Inst. 3, 535 (1932).

L. G. Hoxton, Phys. Rev. 10, 90 (1917); J. Opt. Soc. Am. and Rev. Sci. Inst. 18, 442 (1929); Hoxton and D. W. Mann, Bull. Am. Phys. Soc. 10, 8 (1935). S. Grassmann, Physik. Zeits. 32, 148 (1931). H. Conrad-Billroth, Zeits. f. Inst. 54, 301 (1934).

J. W. Horton, J. Frank. Inst. 216, 749 (1933). I am greatly indebted to Dr. Horton for calling the possibilities of his amplifier to my attention in this connection, and for much valuable advice regarding the electrical circuits used in the line-setting device.

F. W. Sears, J. Opt. Soc. Am. 25, 162 (1935).

A. C. Hardy, J. Opt. Soc. Am. 24, 162 (1934).

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