A common problem in the measurement of photon-count statistics is to estimate the probability density function (PDF) of light intensity from those of photon counts. Considerable recent attention has been focused on this problem in the context of astronomical speckle interferometry, where the statistics of the speckle pattern are used for image reconstructionl. As this problem is typically ill-posed, its direct solution is unstable and requires some regularization procedures. Among them, the algebraic solution with Tichonov's regularization2, asymptotic estimators3, and Pade approximants4 were proposed. We formulate here a different approach to the problem which gives quite acceptable results with reasonable facility.
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