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Testing Model Fit

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Overall measures of Fit. CMIN is distributed as chi square with df=p-q ... In general, a lower chi square to df ratio indicates a betteer fitting model ... – PowerPoint PPT presentation

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Title: Testing Model Fit


1
Testing Model Fit
  • SOC 681
  • James G. Anderson, PhD

2
Assessment of Model Fit
  • Examine the parameter estimates
  • Examine the standard errors and significance of
    the parameter estimates.
  • Examine the squared multiple correlation
    coefficients for the equations
  • Examine the fit statistics
  • Examine the standardized residuals
  • Examine the modification indices

3
Measures of Fit
  • Measures of fit are provided for three models
  • Default Model this is the model that you
    specified
  • Saturated Model This is the most general model
    possible. No constraints are placed on the
    population moments It is guaranteed to fit any
    set of data perfectly.
  • Independence Model The observed variables are
    assumed to be uncorrelated with one another.

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Overall measures of Fit
  • NPAR is the number of parameters being estimated
    (q)
  • CMIN is the minimum value of the discrepancy
    function between the sample covariance matrix and
    the estimated covariance matrix.
  • DF is the number of degrees of freedom and equals
    the p-q
  • pthe number of sample moments
  • q the number of parameters estimated

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Overall measures of Fit
  • CMIN is distributed as chi square with dfp-q
  • P is the probability of getting as large a
    discrepancy with the present sample
  • CMIN/DF is the ratio of the minimum discrepancy
    to degrees of freedom. Values should be close to
    1.0 for correct models.

9
Chi Square ?2
  • Best for models with N75 to N100
  • For Ngt100, chi square is almost always
    significant since the magnitude is affected by
    the sample size
  • Chi square is also affected by the size of
    correlations in the model the larger the
    correlations, the poorer the fit

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Chi Square to df Ratio ?2/df
  • There are no consistent standards for what is
    considered an acceptable model
  • Some authors suggest a ratio of 2 to 1
  • In general, a lower chi square to df ratio
    indicates a betteer fitting model

11
Transforming Chi Square to Z
  • Z ?(2?2) - ?(2df-1)

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CMIN
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RMR, GFI
  • RMR is the Root Mean Square Residual. It is the
    square root of the average amount that the
    sample variances and covariances differ from
    their estimates. Smaller values are better
  • GFI is the Goodness of Fit Index. GFI is between
    0 and 1 where 1 indicates a perfect fit.
    Acceptable values are above 0.90.

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GFI and AGFI (LISREL measures)
  • Values close to .90 reflect a good fit.
  • These indices are affected by sample size and can
    be large for poorly specified models.
  • These are usually not the best measures to use.

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RMR, GFI
  • AGFI is the Adjusted Goodness of Fit Index. It
    takes into account the degrees of freedom
    available for testing the model. Acceptable
    values are above 0.90.
  • PGFI is the Parsimony Goodness of Fit Index. It
    takes into account the degrees of freedom
    available for testing the model. Acceptable
    values are above 0.90.

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RMR, GFI
17
Comparisons to a Baseline Model
  • NFI is the Normed Fit Index. It compares the
    improvement in the minimum discrepancy for the
    specified (default) model to the discrepancy for
    the Independence model. A value of the NFI below
    0.90 indicates that the model can be improved.

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Baseline Comparisons
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Bentler-Bonett Index or Normed Fit Index (NFI)
  • Define null model in which all correlations are
    zero
  • ?2 (Null Model) - ?2 (Proposed Model) ?2
    (Null Model)
  • Value between .90 and .95 is acceptable above
    .95 is good
  • A disadvantage of this index is that the more
    parameters, the larger the index.

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Comparisons to a Baseline Model
  • RFI is the Relative Fit Index This index takes
    the degrees of freedom for the two models into
    account.
  • IFI is the incremental fit index. Values close to
    1.0 indicate a good fit.
  • TLI is the Tucker-Lewis Coefficient and also is
    known as the Bentler-Bonett non-normed fit index
    (NNFI). Values close to 1.0 indicate a good fit.
  • CFI is the Comparative Fit Index and also the
    Relative Noncentrality Iindex (RNI). Values close
    to 1.0 indicate a good fit.

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Tucker Lewis Index or Non-normed Fit Index (NNFI)
  • Value ?2/df(Null Model) - ?2/df(Proposed
    Model) ?2/df(Null Model)
  • If the index is greater than one, it is set to1.
  • Values close to .90 reflects a good model fit.
  • For a given model, a lower chi-square to df ratio
    (as long as it is not less than one) implies a
    better fit.

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Comparative Fit Index (CFI)
  • If D ?2 - df, then
  • D(Null Model) - D(Proposed Model)
  • D(Null Model)
  • If index gt 1, it is set to 1 if index lt0, it is
    set to 0
  • A lower value for D implies a better fit
  • If the CFI lt 1, then it is always greater than
    the TLI
  • The CFI pays a penalty of one for every parameter
    estimated

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Parsimony Adjusted Measures
  • PRATIO is the Parsimony Ratio. It is the number
    of constraints in the model being evaluated as a
    fraction of the number of constraints in the
    independence model.
  • PNFI is the result of applying the PRATIO to the
    NFI.
  • PCFI is the result of applying parsimony
    adjustments to the CFI.

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Parsimony-Adjusted Measures
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Measures Based on the Population Discrepancy
  • NCP is an estimate of the noncentrality parameter
    obtained by fitting a model to the population
    moments rather than to the sample moments.

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NCP
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The Minimum Sample Discrepancy Function
  • FMIN is the minimum value of the discrepancy.

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FMIN
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Root Mean Square Error of Approximation (RMSEA)
  • Value ? (?2/df-1)/(N-1)
  • If ?2 lt df for the model, RMSEA is set to 0
  • Good models have values of lt .05 values of gt .10
    indicate a poor fit.

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PCLOSE
  • PCLOSE is the probability for testing the null
    hypothesis that the population RMSEA is no
    greater than 0.05.

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RMSEA
32
Information Theoretic Measures
  • These indices are composite measures of badness
    of fit and complexity.
  • Simple models that fit well receive low scores.
    Complicated poorly fitting models get high
    scores.
  • These indices are used for model comparison not
    to evaluate a single model.

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AIC
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ECVI
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Akaike Information Criterion (AIC)
  • Value ?2 k(k-1) - 2(df)
  • where k number of variables in the model
  • A better fit is indicated when AIC is smaller
  • Not standardized and not interpreted for a given
    model.
  • For two models estimated from the same data, the
    model with the smaller AIC is preferred.

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Information Theoretic Measures
  • BCC is the Browne-Cudeck Criterion
  • BIC is Bayes Information Criterion.
  • CAIC is the consistent AIC
  • ECVI except for a constant scale factor it is the
    same as AIC.
  • MECVI except for a scale factor is the same as
    the BCC.

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Difference in Chi Square
  • Value X2diff X2 model 1 -X2 model 2
  • DFdiff DF model 1 DFmodel 2

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Miscellaneous Measures
  • HOELTER is the largest sample size for which one
    would acc3ept the hypothesis that a model is
    correct.

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HOELTER
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Hoelter Index
  • Value (N-1)?2(crit) 1
  • ?2
  • Where ?2 (crit) is the critical value for the
    chi-square statistic
  • The index should only be calculated if chi square
    is statistically significant.

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Hoelter Index (2)
  • If the critical value is unknown, can
    approximate (1.645 ?(2df-1) 2 1
  • 2 ?2/ (N-1)
  • For both formulas, one rounds down to the nearest
    integer
  • The index states the sample size at which the chi
    square would not be significant

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Hoelter Index (3)
  • In other words, how small ones sample size would
    have to be for chi square to no longer be
    significant
  • Hoelter Recommends values of at least 200
  • Values lt 75 indicate poor fit

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