We show using Monte Carlo methods that serious systematic error may be introduced in the nonlinear least‐squares (NLLSQ) fitting of Lorentzian line spectra of poor statistical quality or with too few data points in the lines. For such spectra we have found that the NLLSQ estimates of Lorentzian linewidth error are unreliable. This has the result of causing the weighted mean linewidth from several similar spectra to be unequal to the result obtained by adding the spectra together channel by channel and then doing the NLLSQ fit. The problem is illustrated using examples from Mössbauer spectroscopy, however, the results appear to be quite generally relevant in all cases where statistically marginal data are fit with Lorentzian lines.
REFERENCES
1.
2.
L.
Pfeiffer
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4.
An implementation of D. W. Marquardt’s technique (Ref. 5) for nonlinear‐least‐squares estimation adapted for use at Bell Laboratories.
5.
D. W. Marquardt, Share Program Library SDS 309‐01 (1966);
6.
7.
See, for example, A. M. Mood and F. A. Gray bill, Introduction to the Theory of Statistics (McGraw‐Hill, New York, 1963).
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G. J. Perlow, private communication.
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W. C. Davidon, “Variable Metric Method for Minimization,” Argonne National Laboratory Report, ANL 5990 Rev. 2, February 1966.
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D. W. Marquardt, Share Program Library SDA 3094‐01, 16 (1966).
11.
The S observations from the Monte Carlo estimates are ordered by increasing magnitude. For the ith estimate a probability is assigned by These probabilities are then used to determine the quantile according to which can be approximated by a function given in C. Hastings, Jr., Approximations for Digital Computers (Princeton U.P., Princeton, N.J., 1955∥, p. 192. Each ordered observation is then plotted as a function of its corresponding quantile.
For a further explanation of these plots see
M. B.
Wilk
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).
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© 1974 The American Institute of Physics.
1974
The American Institute of Physics
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