disable zoom     view article     reuse permissions
Figure 1
The prior distribution, noiseless posterior distribution and noisy posterior distributions for a GP with covariance 〈f(xi)f(xj)〉 = M5/2(|xi − xj|/4), where Mν(r) is the Matérn function as defined in equation (19)[link]. For each distribution, we draw four random functions (colored lines). The black line represents the mean of each distribution, while the dark- and light-shaded regions represent the 1σ and 2σ intervals, respectively.

Journal logoJOURNAL OF
SYNCHROTRON
RADIATION
ISSN: 1600-5775
Volume 31| Part 6| November 2024| Pages 1446-1456
https://doi.org/10.1107/S1600577524008993
Follow J. Synchrotron Rad.
Sign up for e-alerts
E-alerts
Follow J. Synchrotron Rad. on Twitter
Twitter
Follow us on facebook
Facebook
Sign up for RSS feeds
RSS
We use cookies on our websites, and by using this site you are consenting to them: allow all or manage