LS.whittle.loglik {LSTS} | R Documentation |
Locally Stationary Whittle log-likelihood Function
Description
This function computes Whittle estimator for LS-ARMA and LS-ARFIMA models, in data with mean zero. If mean is not zero, then it is subtracted to data.
Usage
LS.whittle.loglik(
x,
series,
order = c(p = 0, q = 0),
ar.order = NULL,
ma.order = NULL,
sd.order = NULL,
d.order = NULL,
include.d = FALSE,
N = NULL,
S = NULL,
include.taper = TRUE
)
Arguments
x |
(type: numeric) parameter vector. |
series |
(type: numeric) univariate time series. |
order |
(type: numeric) vector corresponding to |
ar.order |
(type: numeric) AR polimonial order. |
ma.order |
(type: numeric) MA polimonial order. |
sd.order |
(type: numeric) polinomial order noise scale factor. |
d.order |
(type: numeric) |
include.d |
(type: numeric) logical argument for |
N |
(type: numeric) value corresponding to the length of the window to
compute periodogram. If |
S |
(type: numeric) value corresponding to the lag with which will go taking the blocks or windows. |
include.taper |
(type: logical) logical argument that by default is
|
Details
The estimation of the time-varying parameters can be carried out by means of the Whittle log-likelihood function proposed by Dahlhaus (1997),
L_n(\theta) = \frac{1}{4\pi}\frac{1}{M} \int_{-\pi}^{\pi}
\bigg\{log f_{\theta}(u_j,\lambda) +
\frac{I_N(u_j, \lambda)}{f_{\theta}(u_j,\lambda)}\bigg\}\,d\lambda
where M
is the number of blocks, N
the length of the series per
block, n =S(M-1)+N
, S
is the shift from block to block,
u_j =t_j/n
, t_j =S(j-1)+N/2
, j =1,\ldots,M
and
\lambda
the Fourier frequencies in the block
(2\,\pi\,k/N
, k = 1,\ldots, N
).
References
For more information on theoretical foundations and estimation methods see Brockwell PJ, Davis RA, Calder MV (2002). Introduction to time series and forecasting, volume 2. Springer. Palma W, Olea R, others (2010). “An efficient estimator for locally stationary Gaussian long-memory processes.” The Annals of Statistics, 38(5), 2958–2997.