1 / 7

T =

Output Y(s). ??. T =. s 3. Input (s). s 1. s P. s 2. n = Number of Input Points (=3) T = Number of Outputs at each input, i.e., “Replications” (=5). Special Cases I’d like to be able to deal with. When T = 1 (i.e., 1 Replication) and assuming normality it should reduce to a GP.

thyra
Download Presentation

T =

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Output Y(s) ?? T = s3 Input (s) s1 sP s2 n = Number of Input Points (=3) T = Number of Outputs at each input, i.e., “Replications” (=5)

  2. Special Cases I’d like to be able to deal with • When T = 1 (i.e., 1 Replication) and assuming normality it should reduce to a GP. • When n = 1 (i.e., 1 input point) it should reduce to CDF estimation as with a univariate DP prior.

  3. Gelfand, Kottas, and MacEachernJASA vol. 100, No. 471 (2005) Output Z(x) Each color is a different replication Input (x) x3 x1 x2

  4. Gelfand, Kottas, and MacEachernJASA vol. 100, No. 471 (2005)

  5. How to break the association of outputs across inputs? • Could add a (uniform?) prior on Replication membership. • This could in principle be dealt with by inserting a Metropolis step within the Gibbs sampler . • I’m unsure whether this Gelfand et al. technique is helpful for estimating the CDF when there is only one input point.

  6. Another Idea • Where CH(f)(F1,…,Fn) is a copula, either: • Elliptically contoured (e.g., Gaussian) • Fairlie-Gumbel-Morgenstern

  7. Copulae • Gaussian • F-G-M

More Related