Paper:	The Shape of Things to Come?
Volume:	371, Statistical Challenges in Modern Astronomy IV
Page:	284
Authors:	Hendry, M.A.
Abstract:	I consider the method of non-parametric shape-restricted estimation, as developed and applied by Woodroofe to the problem of constraining the distribution of Galactic dark matter – an example of an integral deconvolution. I briefly describe several other current problems in astrophysics to which non-parametric shape-restricted estimation and/or integral deconvolution methods are applicable.

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