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324—Appendix B. Command Reference

lambda=arg Set smoothing parameter value to arg; a larger number results in greater smoothing.

power=arg Set smoothing parameter value using the frequency (default=2) power rule of Ravn and Uhlig (2002) (the number of

periods per year divided by 4, raised to the power arg, and multiplied by 1600).

Hodrick and Prescott recommend the value 2; Ravn and

Uhlig recommend the value 4.

If no smoothing option is specified, EViews will use the power rule with a value of 2.

Other Options

pPrint the graph of the smoothed series and the original series.

Examples

gdp.hpf(lambda=1000) gdp_hp

smooths the GDP series with a smoothing parameter “1000” and saves the smoothed series as GDP_HP.

Cross-references

See “Hodrick-Prescott Filter” on page 354 of the User’s Guide for details.

impulse

Var View

 

 

Display impulse response functions of var object with an estimated VAR or VEC.

Syntax

Var View:

var_name.impulse(n, options) ser1 [ser2 ser3 ...] [@ shock_series

 

[@ ordering_series]]

You must specify the number of periods n for which you wish to compute the impulse responses.

List the series names in the var whose responses you would like to compute . You may optionally specify the sources of shocks. To specify the shocks, list the series after an “@”. By default, EViews computes the responses to all possible sources of shocks using the ordering in the Var.

impulse—325

If you are using impulses from the Cholesky factor, you may change the Cholesky ordering by listing the order of the series after a second “@”.

Options

g (default)

Display combined graphs, with impulse responses of

 

one variable to all shocks shown in one graph. If you

 

choose this option, standard error bands will not be dis-

 

played.

 

 

m

Display multiple graphs, with impulse response to each

 

shock shown in separate graphs.

 

 

t

Tabulate the impulse responses.

a

Accumulate the impulse responses.

imp=arg

Type of factorization for the decomposition: unit

(default=“chol”)

impulses, ignoring correlations among the residuals

 

(“imp=unit”), non-orthogonal, ignoring correlations

 

among the residuals (“imp=nonort”), Cholesky with

 

d.f. correction (“imp=chol”), Cholesky without d.f.

 

correction (“imp=mlechol”), Generalized

 

(“imp=gen”), structural (“imp=struct”), or user speci-

 

fied (“imp=user”).

 

The structural factorization is based on the estimated

 

structural VAR. To use this option, you must first esti-

 

mate the structural decomposition; see svar (p. 494).

 

For user-specified impulses, you must specify the name

 

of the vector/matrix containing the impulses using the

 

“fname=” option.

 

The option “imp=mlechol” is provided for backward

 

compatibility with EViews 3.x and earlier.

fname=name

Specify name of vector/matrix containing the impulses.

 

The vector/matrix must have k rows and 1 or k col-

 

umns, where k is the number of endogenous variables.

 

 

326—Appendix B. Command Reference

se=arg

Standard error calculations: “se=a” (analytic),

 

“se=mc” (Monte Carlo).

 

If selecting Monte Carlo, you must specify the number

 

of replications with the “rep=” option.

 

Note the following:

 

(1) Analytic standard errors are currently not available

 

for (a) VECs and (b) structural decompositions identi-

 

fied by long-run restrictions. The “se=a” option will be

 

ignored for these cases.

 

(2) Monte Carlo standard errors are currently not avail-

 

able for (a) VECs and (b) structural decompositions.

 

The “se=mc” option will be ignored for these cases.

 

 

rep=integer

Number of Monte Carlo replications to be used in com-

 

puting the standard errors. Must be used with the

 

“se=mc” option.

 

 

matbys=name

Save responses by shocks (impulses) in named matrix.

 

The first column is the response of the first variable to

 

the first shock, the second column is the response of

 

the second variable to the first shock, and so on.

matbyr=name

Save responses by response series in named matrix.

 

The first column is the response of the first variable to

 

the first shock, the second column is the response of

 

the first variable to the second shock, and so on.

 

 

p

Print the results.

Examples

var var1.ls 1 4 m1 gdp cpi

var1.impulse(10,m) gdp @ m1 gdp cpi

The first line declares and estimates a VAR with three variables. The second line displays multiple graphs of the impulse responses of GDP to shocks to the three series in the VAR using the ordering as specified in VAR1.

var1.impulse(10,m) gdp @ m1 @ cpi gdp m1

displays the impulse response of GDP to a one standard deviation shock in M1 using a different ordering.

jbera—327

Cross-references

See Chapter 24, “Vector Autoregression and Error Correction Models”, on page 719 of the User’s Guide for a discussion of variance decompositions in VARs.

See also decomp (p. 270).

jbera

Var View

 

 

Multivariate residual normality test.

Syntax

 

Var View:

var_name.jbera(options)

You must specify a factorization method using the “factor=” option.

Options

factor=chol

Factorization by the inverse of the Cholesky factor of

 

the residual covariance matrix.

 

 

factor=cor

Factorization by the inverse square root of the residual

 

correlation matrix (Doornik and Hansen, 1994).

 

 

factor=cov

Factorization by the inverse square root of the residual

 

covariance matrix (Urzua, 1997).

 

 

factor=svar

Factorization matrix from structural VAR. You must first

 

estimate the structural factorization to use this option;

 

see svar (p. 494).

 

 

name=arg

Save the test statistics in a named matrix object. See

 

below for a description of the statistics contained in the

 

stored matrix.

 

 

p

Print the test results.

The “name=” option stores the following matrix. Let the VAR have k endogenous variables. Then the stored matrix will have dimension ( k + 1 ) × 4 . The first k rows contain statistics for each orthogonal component, where the first column contains the third moments, the second column contains the χ21 statistics for the third moments, the third column contains the fourth moments, and the fourth column holds the χ21 statistics for the fourth moments. The sum of the second and fourth columns are the Jarque-Bera statistics reported in the last output table.

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