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References

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  1. M. Harwit, P. G. Phillips, T. Fine, N. J. S. Sloane, Appl. Opt. 9, 1149 (1970).
    [CrossRef] [PubMed]
  2. N. J. A. Sloane, T. Fine, P. G. Phillips, M. O. Harwit, Appl. Opt. 8, 2103 (1969).
    [CrossRef] [PubMed]

1970 (1)

1969 (1)

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Figures (1)

Fig. 1
Fig. 1

The first nineteen traces represent a one-dimensional image of the mercury source at various wavelengths centered about 1.7 μ. The bottom trace is an enhanced signal-to-noise spectrum of the same region. The second peak is actually a doublet that cannot be resolved by this instrument. The results are for N2 = 361 measurements.

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