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.

Astronomical Society of the Pacific
Conference Series

© Copyright 1988 - 2025 - Astronomical Society of the Pacific
No part of the material protected by this copyright may be reproduced or used in any form other than for personal use without written permission from the ASP.

Page generated in 0.039 seconds