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Analysis of Lunar Occultation Data
Published online by Cambridge University Press: 30 March 2016
Abstract
The technique of model fitting has been applied to the analysis of data obtained from photoelectric measurements of lunar occultations. A model occultation curve is generated and fitted, by least squares, to the observed light curve, and by this method the values of the model parameters are determined, together with their formal errors. This technique is contrasted with Scheuer’s deconvolution procedure by applying both methods to the same observed data.
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- III. Joint Discussions
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- Copyright © Reidel 1971
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