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    Structural Equation Modeling with AMOS 5.0

    1. Raw data should be saved in SPSS (.sav) format.

    2. Open AMOS Graphicsfrom the Start Menu.

    3. Select New from the File Menu.

    4. Select Data Files from the File Menu. Then click on the File Name button,and use the browser window to locate your SPSS data file.

    5. You can use the View Data button to check your data (it will appear in SPSS).

    6. Click OK to go on.

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    7. Use the List Variables in Dataset button on the left-hand side to see the

    variables in your dataset:

    8. Drag and drop the observed variables that you want to include in your model onto

    the gray workspace:

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    9. Use the oval button on the left to draw in any unobserved (latent) variables that

    you want to include in your model. Double click on the new variable (the ovalyou drew) in order to give it a name. Each variable must be named.

    10.Use the arrow tool on the left to draw paths between variables. The path always

    goes in the direction of latent variable (oval) to observed variable (rectangle).

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    11.Use the double-sided arrow to draw covariances:

    12.Add error variances(residuals) for each observed variable. These are unique,

    unobserved variables for each observed variable. This is an important step, and

    AMOS will give you a warning message and be unable to proceed if you omit it.

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    13.Enter regression weights for each of the relationships between observed and

    unobserved variables. (Unless you have reason to believe that some associations

    will be stronger than others, use 1 for all regression weights. If you believe, e.g.,that one association is 2x as strong as another, use 2 for the weight that is twice as

    strong, and 1 for the other). Note that it is not necessary to specify regression

    weights for everyrelationship. Specify them for each error term, and specify thefirst regression weight for each unobserved to observed variable, as shown below:

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    14.In the View/Set menu, select Analysis Properties. Go to the Output tab.

    Select Standardized Estimates.

    15.Run the model using the calculate estimates button on the left-side controlpanel:

    AMOS stands for Analysis of MOment Structures. AMOS calculates estimates for

    the parameters and fits the model based on mean and covariance structures, to makethese fit the data as closely as possible.

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    16.View the results by clicking on the View Output button. This will show you the

    solution for the model. Select standardized or unstandardized estimates.

    17.Test the model against other plausible models by clicking on the view textbutton to see all statistical outputs from the procedure:

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    18.Notes for Model shows the chi-square statistic that tests for significant

    deviations between the model and the data. In this case, the p-value is significant,

    meaning that the model is not a good fitfor the data (chi-square is used as abadness of fit statistic in SEM).

    Notes for Model (Default model)

    Computation of degrees of freedom (Default model)

    Number of distinct samplemoments:

    55

    Number of distinct parametersto be estimated:

    21

    Degrees of freedom (55 - 21): 34

    Result (Default model)

    Minimum was achieved

    Chi-square = 52.738

    Degrees of freedom = 34

    Probability level = .021

    19.If adequate fit was not achieved, go back and change the model to improve it.

    There are some theoretical reasons (from earlier exploratory factor analysis work)to expect that the Coding subtest was not strongly related to the underlying

    constructs of Verbal and Performance IQ. Therefore, this subtest was deleted

    from the model.

    20.

    In the analysis properties tab, you can select modification indices. This will

    print suggestions in the output for how to improve your model. However, be

    careful to take suggestions only if they make theoretical sense.

    21.This time, the model fits much better (chi square = 38.1,p= .058). Interestingly,

    the paths showing the strongest correlations with the underlying factors(Vocabulary with VIQ and Block Design with PIQ) are the same as those

    suggested in published results for this test and found with exploratory factor

    analysis in other samples. Overall, the results are consistent with the predictedtwo-factor model of intelligence.

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    22.The chi-square does not have to indicate a complete fit in order to accept the model

    with a large sample, the chi-squaresp-value is always likely to be small. Thefollowing alternative fit indices are provided in the text output. AMOS automatically

    compares your model to a saturated model (all variables correlated with all others)and to an independence model (all variables uncorrelated with all others), to ensurethat your model is a better fit. The various fit indices are described below:

    Model Fit Summary

    CMIN

    Model NPAR CMIN DF P CMIN/DF

    Default model 19 38.177 26 .058 1.468

    Saturated model 45 .000 0

    Independence model 9 429.884 36 .000 11.941

    RMR, GFI

    Model RMR GFI AGFI PGFI

    Default model .433 .952 .918 .550

    Saturated model .000 1.000

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    Model RMR GFI AGFI PGFI

    Independence model 2.521 .532 .415 .425

    Baseline Comparisons

    Model NFIDelta1

    RFIrho1

    IFIDelta2

    TLIrho2

    CFI

    Default model .911 .877 .970 .957 .969

    Saturated model 1.000 1.000 1.000

    Independence model .000 .000 .000 .000 .000

    Parsimony-Adjusted Measures

    Model PRATIO PNFI PCFI

    Default model .722 .658 .700

    Saturated model .000 .000 .000

    Independence model 1.000 .000 .000

    NCP

    Model NCP LO 90 HI 90

    Default model 12.177 .000 32.787

    Saturated model .000 .000 .000

    Independence model 393.884 330.800 464.416

    FMIN

    Model FMIN F0 LO 90 HI 90

    Default model .219 .070 .000 .188

    Saturated model .000 .000 .000 .000

    Independence model 2.471 2.264 1.901 2.669

    RMSEA

    Model RMSEA LO 90 HI 90 PCLOSE

    Default model .052 .000 .085 .432

    Independence model .251 .230 .272 .000

    HOELTER

    ModelHOELTER

    .05HOELTER

    .01

    Default model 178 209

    Independence model 21 24

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    CMIN minimum value of the discrepancy between the model and the data.This is the same as the chi-square statistic in the notes for model section.

    CMIN/DF the chi-square divided by its degrees of freedom. Acceptablevalues are in the 3/1 or 2/1 range. Using this criterion, our earlier model

    (without the added path from PIQ to COMP) was also acceptable(CMIN/DF = 1.65)

    RMR, GFI The RMR [Root Mean Square Residual] is the square root ofthe average squared amount by which your models estimated sample

    variances and covariances differ from their actual values in the data. The

    smaller the RMR the better, with RMR = 0 indicating a perfect fit. The GFI[Goodness of Fit Index] is similar to the Baseline Comparisons described

    below, giving a statistic between 0 and 1, with 1 indicating perfect fit, and is

    used with maximum likelihood estimation for missing data. The AGFI

    [Adjusted Goodness of Fit Index] takes into account the degrees of freedomavailable for testing the model (this statistic can have values below zero). The

    PGFI [Parsimony Goodness of Fit Index] is another modification of the GFIthat also takes into account the degrees of freedom available for testing themodel.

    Baseline Comparisons NFI [Normed Fit Index] shows how far between the

    (terribly fitting) independence model and the (perfectly fitting) saturatedmodel the detaulf model is. In this case, its 91% of the way to perfect fit. RFI[Relative Fit Index] is the NFI standardized based on the dfof the models,

    with values close to 1 again indicating a very good fit. IFI [Incremental Fit

    Index], TLI [Tucker-Lewis Coefficient], and CFI [Comparative Fit Index] aresimilar. Note that TLI is usually between 0 and 1, but is not limited to that

    range.

    Parsimony-Adjusted Measures The PRATIO [Parsimony Ratio] is anoverall measure of how parsimonious the model is. It is defined as the dfofthe current model divided by the df of the independence model. It can be

    interpreted as the current model is X% as complex as the independence

    model. The difference between this number and 1 is how much moreefficient your model is than the independence model. PRATIO is used to

    calculate two other statistics: PNFI [Parsimonious Normed Fit Index] is

    another modification of the NFI that takes into account the df(i.e.,complexity) of the model. Similarly, the PCFI [Parsimonious Comparative Fit

    Index] is a df-adjusted modification of the CFI. These two measures are likely

    to be lower than the NFI and CFI, because they take model complexity into

    account. NCP the noncentrality parameter. The columns labeled LO 90 and HI

    90 give the 90% confidence interval for this statistic. This statistic can also

    be interpreted as a chi-square, with the same degrees of freedom as in CMIN.

    FMIN F0 is the noncentrality parameter (NCP) divided by its degrees offreedom. This is similar to the CMIN/DF statistic. The results also give the

    lower and upper limits of a 90% confidence interval for this statistic (LO 90

    and HI 90 under the FMIN heading).

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    RMSEA F0 tends to favor more complex models. RMSEA is a correctedstatistic that gives a penalty for model complexity, calculated as the square

    root of F0 divided by DF (RMSEA stands for root mean squared error of

    approximation). Again, upper and lower bounds of a 90% confidence intervalare given. RMSEA values of .05 or less are good fit, .05 are moderate,

    and .1 or greater are unacceptable. RMSEA = .00 indicates perfect fit. ThePCLOSE statistic that goes with this result is the probability of a hypothesistest that the population RMSEA is no greater than .05 (so, you want this result

    to be nonsignificant [p> .05], because you do not want to prove that the

    RMSEA is significantly greater than .05).

    HOELTER Hoelters criticalN is the largest sample size for which onewould accept the hypothesis that a model is correct (in other words, the

    sample size above which the chi-square goodness of fit test would go from

    nonsignificant to significant). AMOS reports a criticalNfor significancelevels of .05 (which was used by Hoelter) and .01. The result can be

    interpreted as the model would be rejected at the [.05/.01] level with a

    sample size of greater than X. Hoelter suggests that models which would berejected only with 200 or more participants (a number of 200 or higher in the

    Hoelter section of the output) are an adequate fit for the data. Numbers

    smaller than 200 suggest an inadequate fit. Arbuckle disagrees with the use of

    this criterion, and its not one of the more commonly reported statistics forSEM, but other experts may use it.

    The remaining measures are intended for comparing multiple models, rather thanevaluating goodness of fit for a single model:

    AIC

    Model AIC BCC BIC CAIC

    Default model 76.177 78.494 136.308 155.308

    Saturated model 90.000 95.488 232.415 277.415

    Independence model 447.884 448.981 476.367 485.367

    ECVI

    Model ECVI LO 90 HI 90 MECVI

    Default model .438 .368 .556 .451

    Saturated model .517 .517 .517 .549

    Independence model 2.574 2.211 2.979 2.580

    AIC the Akaike Information Criterion is calculated as the discrepancy (C) +2q(a complexity statistic).

    BCC the Browne-Cudeck Criterion imposes a slightly greater penalty for

    model complexity than the AIC does. Arbuckle (author of the AMOS

    program) recommends this particular fit index.

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    BIC the Bayesian Information Criterion assigns an even greater penalty forcomplexity, and therefore has a tendency to choose parsimonious models.

    This can only be used in single-group models.

    CAIC the Consistent AIC has a greater penalty for complexity than AIC orBCC, but not as much as BIC does. Can only be used in single-group models.

    ECVI Arbuckle reports that except for a constant scale factor, ECVI[expected cross-validation index] is the same as AIC (it is equal to AIC / n).

    Upper and lower 90% confidence interval limits are also given for ECVI.

    MECVI is similar, equal to BCC / n. When maximum likelihood estimation

    has been used to compensate for missing data, Arbuckle provides a

    recommendation to use MECVI instead of ECVI.

    23.Specification Search options An extra feature in AMOS 5.0 is the ability to do a

    specification search. This feature allows you to test various models simultaneously,

    by specifying that some relationships between variables are optional. For instance,what if I wanted to test the different fit obtained by using a model with two correlated

    factors of IQ versus two uncorrelated factors? I could use the Specification Searchcommand in the Model-Fit menu.

    a. To see the optional relationships correctly, first go to the View-Set

    menu and select Interface Properties:

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    b. On the Accessibility tab, check the alternative to color checkbox. This

    will cause optional relationships between variables to show up as dashed

    lines on the path diagram (rather than just showing up in blue, which isharder to see):

    c. Open the Specification Search toolbar using the binoculars tool:

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    d. Use the dashed-arrow tool to make some relationships between variables

    optional components of the model. Just click on the tool, then click on the

    relationship to be changed. You can reverse this action if necessary byusing the solid-line tool thats just to the right on the toolbar.

    e. Run the specification search using the arrow tool on the toolbar. An outputsection will appear in the toolbar itself, showing results for each model:

    f. You can interpret models using the chi-square andp-values provided, or

    you can see more details. If you double click on one of the lines in this

    window, or select it and then use the blue-box tool on the toolbar, you willsee the actual path diagram to know which of the optional components

    have been included or omitted. In this case, Model 2 has a higherp-value

    (which you want with SEM), and includes the VIQ-PIQ covariance.

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    g. If you got a lot of options, AMOS has a view short list button on the

    toolbar to help you sift through them.

    h. To see RMSEA and other statistics, use the checkbox icon on the toolbar,

    and under the Current Results tab, check the box for Derived fit

    indices in the Display section. Also, if you select Akaike weights inthe lower section of this menu, you can get a statistic in the BCC

    column that can be interpreted as the likelihood of the model given the

    data. This is a useful way to compare models. The model with the smallestvalue here (or the lowest BIC value originally) is the best fit for the data.

    i. You can also see comparisons between models graphically, using the

    Plots button on the toolbar. Select Best Fit and AIC or BIC.BCC is also possible, but imposes a greater penalty for complexity.

    This graph shows you fit (on theyaxis) vs. complexity (on thexaxis), wth

    the lowestyvalue showing you the best fit vs. complexity ratio. Click on

    the individual data point, and AMOS will tell you which model numberwas selected. Click on that model in the output window to see the model.