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| 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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