Gretl
Jan 18, 2021 Gretl will access other available versions on demand, via the Internet. You can also find the manual files here. Avid port devices driver download. In addition the Gretl Command Reference and Gretl Function Reference are available in HTML format. Fujifilm driver download for windows 10. Getting help, reporting bugs. If you use gretl you may wish to join the gretl-users mailing list. This is a moderate-volume list where. Gretl commands 1.1 Introduction The commands defined below may be executed interactively in the command-line client program or in the console window of the GUI program. They may also be placed in a “script” or batch file for non-interactive execution. The following notational conventions are used below. Witchslayer Gretl (also known as Gretl and Gretl: Witch Hunter) is a 2012 American-Canadian dark fantasy television film written by Brook Durham and Angela Mancuso, and directed by Mario Philip Azzopardi. Microage college station driver download for windows 10.
I use some quarterly inflation series from the Stock/Watson textbook for which the dataset is already provided by gretl:
<hansl>
set verbose off
open sw_ch14.gdt -q
series x = ldiff(PUNEW) # construct quarterly CPI inflation
</hansl>
2) Obtain fitted values = 1-step ahead forecasts
<hansl>
ols x const x(-1) -q# Estimate the AR(1) by OLS
series yhat = $yhat# Grab the fitted value by the built-in accesor $yhat
fcast fit# Alternatively one can use
print x fit yhat -o# Compare the results
</hansl>
In this exercise, the training set consists of the first R observations to fit a model. We take the coefficient vector beta-hat as given, and fit the model to a test set consisting R+1 to T observations of actual realizations.
<hansl>
smpl ; 1989:4# set the training set
ols x 0 x(-1)# estimate the AR(1) model
scalar fc1990q1 = bhat[1] + x[1989:4]*bhat[2]
scalar fc1990q2 = bhat[1] + x[1990:1]*bhat[2]
scalar fc1990q3 = bhat[1] + x[1990:2]*bhat[2]
print fc1990q1 fc1990q2 fc1990q3
# 1990q1 and 1990q3 using gretl's 'fcast' command
# We can also do this for all periods after 1999m12
# Note that you don't have to specify a concrete date
# but could just move the period forecasted by
fcast ($t2+1) ($t2+3) --static
</hansl>
<hansl>
smpl ; 1989:4# set the training set
ols x 0 x(-1)# estimate the AR(1) model
matrix bhat = $coeff# grab the coefficient vector
# Do the dynamic forecast by hand first
scalar dfc1990q1 = bhat[1] + x[1989:4]*bhat[2]# 1st value is the actual outcome
scalar dfc1990q2 = bhat[1] + dfc1990q1*bhat[2]# now we use the forecasted value of the previous period
scalar dfc1990q3 = bhat[1] + dfc1990q2*bhat[2]
print dfc1990q1 dfc1990q2 dfc1990q3
# Compare using gretl
fcast 1990:1 1990:3 --dynamic
# Run the dynamic forecast for all remaining periods
fcast --dynamic --out-of-sample
</hansl>
smpl full
ols x 0 x(-1) -q
fcast 1990:1 1990:2 1 --rolling# 1-step ahead rolling fc
# Compare fc for 1990:2 with
smpl full
smpl ; 1990:1
ols x 0 x(-1) -q
fcast ($t2+1) ($t2+1) --dynamic
# or equivalently
fcast ($t2) ($t2+1) --static
smpl full
ols x 0 x(-1) -q
fcast 1 fc1 --rolling# 1-step ahead
fcast 6 fc6 --rolling# 6-step ahead
gnuplot x fc1 fc6 --with-lines --time-series --output=display
I use some quarterly inflation series from the Stock/Watson textbook for which the dataset is already provided by gretl:
<hansl>
set verbose off
open sw_ch14.gdt -q
series x = ldiff(PUNEW) # construct quarterly CPI inflation
</hansl>
2) Obtain fitted values = 1-step ahead forecasts
<hansl>
ols x const x(-1) -q# Estimate the AR(1) by OLS
series yhat = $yhat# Grab the fitted value by the built-in accesor $yhat
fcast fit# Alternatively one can use
print x fit yhat -o# Compare the results
</hansl>
In this exercise, the training set consists of the first R observations to fit a model. We take the coefficient vector beta-hat as given, and fit the model to a test set consisting R+1 to T observations of actual realizations.
<hansl>
smpl ; 1989:4# set the training set
ols x 0 x(-1)# estimate the AR(1) model
scalar fc1990q1 = bhat[1] + x[1989:4]*bhat[2]
scalar fc1990q2 = bhat[1] + x[1990:1]*bhat[2]
scalar fc1990q3 = bhat[1] + x[1990:2]*bhat[2]
print fc1990q1 fc1990q2 fc1990q3
# 1990q1 and 1990q3 using gretl's 'fcast' command
# We can also do this for all periods after 1999m12
# Note that you don't have to specify a concrete date
# but could just move the period forecasted by
fcast ($t2+1) ($t2+3) --static
</hansl>
Witchslayer Gretl
In this case, we estimate the model using the first R observations as our training set, again grab the coefficient vector beta-hat, and fit the model to the following R+h observations. However, instead of using actual realizations of x, we use the forecasted values. Thus, one obtains for the h-step ahead forecast (e.g. h=2) a whole path of forecasts.Gretl Crawford Homes
<hansl>smpl ; 1989:4# set the training set
ols x 0 x(-1)# estimate the AR(1) model
matrix bhat = $coeff# grab the coefficient vector
# Do the dynamic forecast by hand first
scalar dfc1990q1 = bhat[1] + x[1989:4]*bhat[2]# 1st value is the actual outcome
scalar dfc1990q2 = bhat[1] + dfc1990q1*bhat[2]# now we use the forecasted value of the previous period
scalar dfc1990q3 = bhat[1] + dfc1990q2*bhat[2]
print dfc1990q1 dfc1990q2 dfc1990q3
# Compare using gretl
fcast 1990:1 1990:3 --dynamic
# Run the dynamic forecast for all remaining periods
fcast --dynamic --out-of-sample
</hansl>
Gretl Download
smpl full
ols x 0 x(-1) -q
fcast 1990:1 1990:2 1 --rolling# 1-step ahead rolling fc
# Compare fc for 1990:2 with
smpl full
smpl ; 1990:1
ols x 0 x(-1) -q
fcast ($t2+1) ($t2+1) --dynamic
# or equivalently
fcast ($t2) ($t2+1) --static
smpl full
ols x 0 x(-1) -q
fcast 1 fc1 --rolling# 1-step ahead
fcast 6 fc6 --rolling# 6-step ahead
gnuplot x fc1 fc6 --with-lines --time-series --output=display