Skip to content

Commit

Permalink
minor
Browse files Browse the repository at this point in the history
  • Loading branch information
lionelvoirol committed Nov 15, 2024
1 parent 96995f5 commit e2c830d
Show file tree
Hide file tree
Showing 2 changed files with 4 additions and 2 deletions.
4 changes: 3 additions & 1 deletion README.md
Original file line number Diff line number Diff line change
@@ -1,4 +1,6 @@
# `gmwmx2` Overview <img src="man/figures/logo.png" align="right" style="width: 20%; height: 20%"/>
# `gmwmx2` Overview <img src="man/figures/logo.png" align="right" style="width: 15%; height: 15%"/>



The `gmwmx2` `R` package implements the Generalized Method of Wavelet Moments with Exogenous Inputs estimator (GMWMX) presented in [Voirol, L., Xu, H., Zhang, Y., Insolia, L., Molinari, R. and Guerrier, S. (2024)](https://arxiv.org/abs/2409.05160).
The GMWMX estimator is a computationally efficient estimator to estimate large scale regression problems with complex dependence structure in presence of missing data.
Expand Down
2 changes: 1 addition & 1 deletion vignettes/fit_model.Rmd
Original file line number Diff line number Diff line change
Expand Up @@ -139,7 +139,7 @@ $$
$$
When the argument `stochastic_model` is set to `"wn + pl"`, the stochastic model considered includes both white noise and colored noise with the specified above autocovariance structure. The model is therefore stationary and the parameters estimated are: $\sigma^2_{W N}$, $\kappa$ (constrained to be greater than $-1$) and $\sigma^2_{P L}$.

When the argument `stochastic_model` is set to `"wn + fl"`, the stochastic model considered includes both white noise and flicker noise (not stationary power-law noise with spectral index $\kappa=-1$) where the variance covariance of the flicker noise $\omega$ is obtained as follows (see e.g., [@bos2008fast]):
When the argument `stochastic_model` is set to `"wn + fl"`, the stochastic model considered includes both white noise and flicker noise (not stationary power-law noise with spectral index $\kappa=-1$) where the variance covariance of the flicker noise $\omega$ is obtained as follows (see e.g., [@bos2008fast]):

$$
\operatorname{Cov}(\omega) = \sigma^2_{F L}\mathbf{U}^T \mathbf{U}
Expand Down

0 comments on commit e2c830d

Please sign in to comment.