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Psicothema, 1994. Vol. Vol. 6 (nº 2). 297-310

Alberto Maydeu-Olivares

University of Illinois

Latent trait models (LTMs) are one type of individual differences scaling models. Most commonly, these models use parametric functions to model the option response functions (ORFs) and latent trait distributions, although recently several nonparametric LTMs have also been proposed. In this paper, the strengths of each of these two approaches are discussed by comparing two models: Muthén's parametric LISCOMP model, and Levine's nonparametric MFS model. It was found that the MFS model is particularly suited for unidimensional scaling since it allows density estimation, it is more flexible at modeling the shape of the ORFs, and therefore may be more robust to mispecifications of the dimensionality of the data. The LISCOMP model, on the other hand, is particularly suited for multidimensional scaling, and for modeling the relationships between the scaling dimensions and external variables. Nonparametric models such as MFS are not easily generalized to multidimensional situations since they usually rely on smoothing constraints to reduce the estimation parameter space. These constraints are based on assumptions about the functional form of the ORFs and the latent trait densities, and it may be difficult to arrive at a set of constraints that will prove appropriate for different sampling schemes and dimensionality hypotheses.

**Key words:** IRT; item response theory.

*Enfoques parametricos versus no parametricos para el escalamiento
de diferencias individuales.* Los modelos de rasgos latentes (MRLs) son un
tipo de modelos de escalamiento de diferencias individuales. Habitualmente,
estos modelos utilizan funciones paramétricas para modelar las funciones
de respuesta a las opciones (FROs) y las distribuciones de los rasgos latentes,
aunque recientemente varios MRLs no paramétricos han sido propuestos.
En este artículo se comparan las ventajas de cada uno de estos dos enfoques
mediante la comparación de dos modelos: el modelo paramétrico
LISCOMP de Muthén, y el modelo no paramétrico MFS de Levine. El
modelo MFS es particularmente apropiado en escalamiento unidimensional dado
que permite estimar la densidad del rasgo latente, es m.s flexible para modelar
las FROs, y como resultado puede ser m.s robusto a mis especificaciones de la
dimensionalidad de los datos. El modelo LISCOMP, por su parte, es particularmente
apropiado en escalamiento multidimensional, así como para modelar las
relaciones entre las dimensiones del escalamiento y variables externas. Los
modelos no paramétricos como MFS no son generalizables fácilmente
a situaciones multidimensionales ya que habitualmente utilizan restricciones
que suavizan la forma de las funciones utilizadas. Estas restricciones se basan
en supuestos acerca de las formas de las FROs y de las densidades de los rasgos
latentes. Sin embargo, puede ser difícil el llegar a establecer un conjunto
de restricciones común para diferentes diseños muestrales y para
diferentes soluciones dimensionales.

**Palabras clave:** TRI; teoría de respuesta a los
items.

One of the main objectives of Psychology as a Science is to
study how we represent our perceptions of stimuli. Different sampling as a Science
is to study how we represent our designs can be used in this endeavor: paired
comparisons, sorting tasks, etc. For simplicity, this article focuses on one
of the most common sampling designs: *the direct response design*. In this
sampling design, which is widely used when the stimuli to be scaled are statements
reflecting values or attitudes, or containing behavioral or cognitive descriptions,
each subject is presented every stimulus one at a time. A forced choice categorical
response format (dichotomous or polychotomous) is commonly presented to the
subjects when this type of stimuli are used. In a dichotomous response format
the subject might be asked, for instance: (a) to endorse or reject a statement
that reflects his/her attitudes, or (2) to check a psychological symptom as
present or absent. In a polychotomous response format the subject might be asked,
for instance: (a) to endorse an attitudinal statement in a rating scale ranging
from strongly disagree to strongly agree, or (b) to rate the occurrence of a
behavior from very infrequent to very frequent. In this context, scaling can
be defined as the mapping of all respondents and stimuli in a continuum, based
on the subjects' categorical responses.

One approach to scaling consists of assuming that all subjects perceive the stimuli in the same way. When this assumption is adequate, we can readily rank order our stimuli along a continuum using appropriate models (e.g., Thurstone, 1927; Coombs, 1950; Bradley & Terry, 1952; Luce, 1959). Alternatively, we may assume that within a homogeneous set of stimuli there are no inter-stimuli differences, and that the observed variability in how subjects respond to stimuli is solely due to systematic individual differences. When this assumption is adequate, the subjects can be rank ordered along a continuum. An example of this approach is given by Likert (1932).

However, it seems more reasonable to believe that the observed variability in the subjects' responses is due to systematic individual differences and to inter-stimuli differences. In that case, it is necessary to find a way to separate the within-individual variability from the between-individual variability. One way to account for the dependencies among observations due to the between-subject variation is to use a statistical model that includes subject parameters along with stimuli parameters. These parameters can then be estimated by asymptotically optimal estimation methods such as maximum likelihood or generalized least squares. Unfortunately, because the subject parameters increase as sample size increases, the desirable asymptotic properties of those estimators do not hold (Neyman & Scott, 1948). One way of solving this problem is to introduce the subject parameters as a random effect, while keeping the stimuli parameters as a fixed effect.

Generally speaking, the probability of observing a vector of categorical responses υ = u can be expressed as

(1) Prob (υ =** u**) = ƒ Prob (υ =
**u** Ι θ = **t**) f (** t** ) d ( **t** )

where f ( **t **) is the probability density function of
the subject parameters and Prob ( υ = **u** Ι θ = **t**
) is the probability of observing a response vector υ = **u** in
a group of subjects with a fixed value, θ =** t**, in the continuum
of subject parameters.

This paper focuses in a subset of the individual differences
scaling models, namely, in those models where the Prob (υ = **u**
Ι θ = **t **) can be represented as

(2) Prob (υ =** u ** Ι θ =** t**)
= Π Prob (υ

where θ is a* q *dimensional vector of subject parameters.
These models are generally called *latent trait models*, and, the random
variables θ (theta) are called *latent traits.* These models have
been most commonly used to scale direct response data, although they may also
well be used to scale data obtained through other sampling designs (see Takane,
1989).

Note that of the three terms appearing in Equation 1, { Prob
( υ = **u **), Prob (υ = **u** Ι θ =** t **),
and f( **t** ) }, generally only one, Prob (υ = **u**), may be
estimated directly and that Prob (υ = **u** Ι θ = **t**
) and f( **t** ) can not be estimated simultaneously (see Bartholomew, 1987).
In any case, it is possible to:

(1) Estimate the function Prob(υ = **u** Ι θ= **t**
) if f ( **t** ) is known (or assumed to be known);

(2) Estimate the density f (**t**) if the function Prob (υ = **u ** Ι
θ= **t **) is known (or assumed to be known); or

(3) Estimate Prob (υ = **u **Ι θ = **t**
) and f (**t**) alternatively. For instance, a) assigning an initial value
to f **(t**) to estimate Prob (υ = **u **Ι θ = **t**),
b) re-estimating f (**t**) using the Prob (υ = **u **Ι θ
= **t**) estimated previously, and so on until the algorithm converges.

Most latent trait models specify an a priori parametric form
for Prob (υ = **u **Ι θ = **t**), usually a cumulative
normal or logistic function, and a parametric function for f (**t**), usually
a normal density. Recently, however, several *non* parametric latent trait
models have been proposed (Ramsey, 1988; Ramsey & Winsberg, 1991; Samejima,
1983, 1988; Levine, 1984; Levine, Drasgow, Williams, Maydeu-Olivares, Mead,
Thomasson, Tsien. Wei, & Zickar, 1993). In this paper these two approaches
will be compared. With this aim, I will describe with some detail (1) a parametric
model of individual differences scaling, proposed by Muthén (1983, 1984,
1987), and (2) a *non *parametric model of individual differences scaling,
proposed by Levine (1984, 1989; Levine* et al*., 1993; Williams & Levine,
1993). To illustrate the exposition, an application of these two approaches
to a set of actual data will be presented.

**PARAMETRIC VS. NON PARAMETRIC LATENT TRAIT MODELS**

In his pioneering work on scaling, Thurstone was already concerned
with the sampling theory foundations of his model. In fact, Thurstone (1927)
introduced two explanations for the nature of the stochasticity of what he referred
to as ‘discriminal processes' of the subjects. These are the Case I and Case
II of this Law of Comparative Judgment. Interestingly enough, Thurstone's case
I and Case II closely match the *stochastic subject rationale and the random
sampling rationale *for latent trait models described by Holland (1990).

Indeed, Holland (1990) has argued that when the data is collected
using a direct response sampling design and fitted by a latent trait model,
the basis for statistical inference lies in what he refers to as a random sampling
rationale. According to this rationale, the meaningfulness of statistical inference
in latent trait models is granted by assuming that: 1) the stimuli are fixed
in the sense of not being sampled, and 2) the subjects are a random sample from
a population. Furthermore, Holland (1990: p. 584) states «I believe that no
completely satisfactory justification of the *stochastic subject *is possible».

If, following Holland (1990), we accept that statistical inference
in latent trait models only requires these two assumptions, then any function
can be used to represent Prob (υ = **u **Ι θ = **t**)
and f (**t**) provided that Equation 2 is satisfied. That is, the density
f(**t**) is only determined up to a choice of the function Prob (υ
= **u **Ι θ = **t**), and vice versa.

The random sampling rationale also has implications for estimation. If the categorical responses to be scaled are obtained from a random sample of subjects from a much larger population, then the maximum likelihood estimator of the log-likelihood of the data is exactly the so called ‘marginal' maximum estimator (MMLE) applied by Bock and Aitkin (1981) to parametric models and by Levine (1989) to nonparametric models (see Holland, 1990: p. 593).

LISCOMP: *A parametric model of individual differences scaling
by covariance structure analysis*

Takane and de Leeuw (1987) and Takane (1989) have shown that many scaling models (e.g. Thurstone, 1927, 1959; Takane, 1980; Heiser & de Leeuw, 1981; De Soete & Carroll, 1983; De Soete, Carroll & DeSarbo, 1986) can be considered as special cases of analysis of covariance structures (ACOVS: Jöreskog, 1970). In particular, Takane and de Leeuw (1987) have shown that most parametric latent trait models for direct response data (e.g. Samejima, 1969; Bock, 1972; Muthén, 1984) are special cases of covariance structures analysis, or more generally, of moment structures analysis, and therefore suitable to be estimated using existing covariance structures software such as LISCOMP (Muthén, 1987) or LISREL 7 (Jöreskog & Sörbom, 1989).

Muthén (1983, 1984, 1987) has described a covariance structures model given by

(3) **y** = υ + Λ θ + ε

(4) θ = α + Bθ + ζ

where θ is a vector of individual differences parameters
(latent traits); Λ and B are matrices of structural and measurement regression
coefficients, respectively; ζ and ε are vectors of structural and
measurement residuals, respectively; and α and υ are vectors of
structural and measurement intercepts, respectively. Categorical ratings, u_{i}
= 1, 2, ..., *k,* ..., *m*, obtained by a direct response design can
be incorporated into the model by assuming that the y variables in Equation
3 have been categorized by

If, in addition, it is assumed that the y and θ variables follow a multinormal distribution we have

(6)

where the τ variables are thresholds, and F(•) is a normal cumulative function. Muthén's (1983, 1984) model is formally equivalent (in the unidimensional case) to Samejima's (1969) graded model (see Takane & de Leeuw, 1987), and is directly related to Thurstonian scaling models (see Thurstone, 1959).

Muthén (1984, 1987) has proposed a thee-stage limited
information estimator of this model that uses only first and second moments
of the data. The resulting weighted least squares loss function is asymptotically
distributed as chi-square with n(n+1)/2-p degrees of freedom, where* p*
is the number of stimuli parameters in the model, and *n* is the number
of stimuli to be analyzed. This weighted least squares estimator must be regarded
as an approximation to the MMLE estimator described by Bock and Aitkin (1981).

*MFS. A non parametric model of individual differences scaling*

There are several non-parametric models of individual differences
scaling (see Levine et al., 1993). In this paper, we will describe only one
of them, Levine's Multilinear Formula Score model (MFS: Levine, 1984, 1989;
Levine *et al*., 1993). The theoretical base of MFS lies on the finiteness
of the span of the posterior densities of the subject parameters (see Levine,
1984, 1992). Since there are finitely many posterior densities, their linear
span forms a finite dimensional vector space. The function corresponding to
any single Prob (ui = k Ι θ=t) is then represented as a linear combination
of a set of basis functions for that span, that is

where h_{j} (t), j = 1, ..., J is an orthogonal basis
function for the span of the posterior densities of the subject parameters,
and a _{j,i,k } is its corresponding coefficient estimated from the
data. Thus, the sample likelihood of Prob (u_{i}=k Ι θ =
t) is evaluated as a function for the unknown coefficients a_{j,i,k.}
The orthogonal basis h_{j }(t) are obtained by a procedure analogous
to principal components performed on the span of the posterior densities of
the subject parameters (Levine, 1989).

Levine* et al.* (1993) have pointed out that the fundamental
feature that distinguishes non parametric from parametric models is that parametric
models use only one function to fit the whole continuum of subject parameters
(the latent trait), whereas non parametric models use an strategy to divide
that continuum into small regions, and then use different functions to model
each one of these subdivisions.

It is also noteworthy to point out that the LISCOMP model uses
the first of the estimation strategies for latent trait models described previously.
That is, the f(t) and Prob( u_{i} = k Ι θ = t ) in this model
are estimated by assuming that f(t) is a multivariate normal distribution, and
that Prob (u_{i}= k Ι θ = t) is a normal cumulative function.

The MFS model uses the third of such estimation strategies:
Initial values of Prob (u_{i} = k Ι θ = t) are used to estimate
by marginal maximum likelihood f(t). Then, a set of orthonormal bases for f(t)
is obtained, h_{j} (t), and the coefficients a_{j,i,k} in Equation
7 are estimated also by marginal maximum likelihood, completing an estimation
cycle. Finally, to improve efficiency of the estimation, constraints are introduced
over specified regions of h based on assumptions about the shapes of the functions
Prob (u_{i} = k Ι θ= t). These constraints reduce the parameter
space by imposing linear inequalities that the vector of coefficients a_{j,i,k}
must satisfy. Three types of constraints are generally imposed: monotonicity
constraints, concavity constraints, and smoothing constraints. Further details
can be found in Levine (1984, 1989, 1992).

Any function Prob (u_{i}= k Ι θ = t) may
be used as starting values of the estimation process. For instance, a regression
of each of the stimuli on some sort of total score of the stimuli can be used
as starting values for MFS. These so-called item-score regressions are obtained
using Sympson's (1988) POLYSCORE procedure. In this paper we used the functions
Prob (u_{i}= k Ι θ = t) estimated by LISCOMP as starting values
for the program FORSCORE (Williams & Levine, 1993) to show how MFS is able
to depart from a good starting value.

*An example*

The five statements that compose the Positive Problem Orientation (PPO) of the Social Problem Solving Inventory -Revised (SPSI-R: D'Zurilla & Maydeu-Olivares, 1993) were scaled using Muthén's (1984) parametric model, and Levine's (1984) non parametric model using the responses of 1053 subjects. Each of the subjects was asked to rate on a five point scale from ‘very true of me' to ‘not at all true of me' the accuracy of each of these five statements in relation to their overall daily behavior and cognitions in real life problem solving. These statements include behaviors that reflect a positive problem appraisal, commitment to a problem-solving coping strategy, problem solving self-efficacy self-expectancies, and positive outcome expectancies when facing real-life problems.

Muthén's (1984) version of Thurstonian scaling was fitted by weighted least squares using LISCOMP (Muthén, 1987). This model did not fit the data very well as assessed by the chi-square goodness-of-fit index χ^{2} (5) = 25.07, p < .001. However, the robustness of this test statistic to violations of the model assumptions when the response variables are categorical have not been extensively studied. Other goodness of fit indices reveal a reasonable good fit of this model: root mean square residual (RMSR)=.034, Tanaka and Huba's (1985) goodness of fit index (GFI)=.994, McDonald's (1988) mk=.991.

The non parametric model MFS was fitted to these data using
the FORSCORE (Williams & Levine, 1993) computer program with 20 estimation
cycles. We used as starting values the functions Prob (u_{i}= k Ι
θ= t) estimated by LISCOMP instead of the POLYSCORE curves to show how
MFS is able to depart from a good parametric starting value.

The marginal maximum likelihood estimation method used by this
program leads to a discrepancy function that is asymptotically distributed as
chi-square with (m^{n}-p) degrees of freedom, where *m* is the
number of response options to each of the stimuli, *n* is the number of
stimuli, and *p* is the number of stimuli parameters. This discrepancy
function is based on the ratio of the likelihood under the fitted model to the
likelihood of a saturated model in which we fit the multinomial distribution
to the empirical frequencies (see McDonald & Mok, 1993). This statistic
can hardly ever be used in practice, since often there are not enough data to
estimate the empirical frequencies of all possible mn response patterns. In
our example, there are 5^{5}=3125 possible response patterns, whereas
only 1053 subject responses are available. Therefore, we are clearly unable
to estimate the empirical frequencies of all possible response patterns.

Drasgow, Levine, Tsien, Williams, and Mead (in press) have
suggested assessing the goodness of fit of these models by inspecting all first
order, second order, and third order chi-square statistics of the m^{n}
table, instead of inspecting the overall m^{n} table, because the empirical
frequencies of these lower order statistics can be readily be estimated.

A chi-square statistic for a single stimulus is obtained by

(8)

where the expected proportions are obtained from

(9)

The chi-square statistics for a pair of stimuli (i,j) are obtained as in Equation 8, but the sum is over pairs of options (k, k') and the expected proportions are obtained by

(10)

The chi-square statistics for a triplet of stimuli are obtained
by the obvious extension of the above procedure (for more details see Drasgow
*et al*., in press).

Since in practice sometimes some of the options are not chosen
by any subject in the sample, these chi-square statistics may have different
degrees of freedom. For this reason, Drasgow* et al.* (in press) recommend
inspecting the ratio chi-square to degrees of freedom to assess the goodness
of fit of the model. In Table 1 I present the results obtained by fitting the
LISCOMP and MFS models to the data of this example. As it can be observed in
this table, all chi-square to degrees of freedom ratios for the MFS model are
less than one, whereas only the chi-square/d.f. ratios for single stimuli are
less than one in the LISCOMP model. Furthermore, the mean of the ratios obtained
from single stimuli for the LISCOMP model (
= .00515) is less than the one obtained for the MFS model (
= .10756). Thus, LISCOMP fits the first order marginals of these data better
than MFS, but MFS provides a better overall fit to the data.

That LISCOMP fits better than MFS the first order marginals
can also be observed graphically by plotting the estimated functions Prob (u_{i}=
k Ι θ = t). In Figures 1 to 4 I present plots of these functions
for the worse fitted stimulus (Figures 1 and 2) and better fitted stimulus (Figures
3 and 4). The vertical lines drawn in these figures correspond to 95% confidence
intervals computed around 25 points in the θ scale (further details on
the construction of these plots can be found in Drasgow *et al., *in press).

Those points where vertical lines have not been drawn indicate that less than five subjects chose that particular option, and therefore, confidence intervals around that point were not computed. In Figures 2 and 4 (corresponding to the MFS model), the estimated density has been transformed to a standard normal density so as to be able to compare these figures with those corresponding to the LISCOMP model.

The inspection of these figures reveals that both models fit
these data satisfactorily. Note, however, that even after transforming its density,
the MFS curves do not resemble the smoother LISCOMP curves. Levine et al. (1993)
have performed several simulation studies that indicate that the somehow strange
forms of the Prob (u_{i}= k Ι θ =t) functions estimated by
MFS are not due to sampling variations, but are due to the existence of multidimensionality
or nonnormal densities in the data. It is precisely the higher flexibility of
MFS to capture small degrees of multidimensionality and to model non normal
densities which allows this model to fit the data of this example better than
the LISCOMP model. In Figure 5, I present a plot of the density of the latent
trait as estimated by MFS. As it can be observed in this figure, the estimated
density is slightly bimodal and most subjects in this sample lie between -1
< θ < 1 . The elevations of the density at the extremes of the graph
(θ ≥ Ι 2 Ι ) are due to the lack of subjects in the extremes of the
distribution, and can be removed by imposing stricter smoothing constrains in
the tails of the distribution.

**CONCLUSIONS**

A large set of scaling models hypothesize that the variability with which subjects perceive, discriminate, and choose among stimuli is due to both inter-individual variability and within-individual variability. These models, referred to as individual differences scaling models, generally use subject as well as stimuli parameters. A subset of the individual differences scaling models are the so-called latent trait models. An examination of the basis for statistical inference of latent trait models reveals that there is no need to postulate any particular functional form for the probability of discriminating or choosing a particular object given a fixed level of the continuum being measured. Thus, the use of nonparametric or semi-parametric latent trait models is fully justifiable. Indeed, in applications (as in the example presented in this paper) non-parametric latent trait models can offer a better fit than parametric latent trait models because.

a) they may be more robust than parametric models to mispecifications of the dimensionality of the data,

b) they are more flexible to model the probability of discriminating or choosing an stimulus,

c) they allow us to estimate a non parametric density of the subject parameters.

A major drawback of these models is that they rely on smoothing constraints to reduce the parameter space of estimation. These constraints are based on assumptions about the functional form of the probability of discriminating or choosing an stimulus given a fixed level of the scaling continuum. However, if these type of models are to be used in multidimensional situations, or with different sampling designs, then it will be necessary to modify the set of smoothing constraints, and it may be difficult to arrive at a set of constraints that will prove appropriate for each of these situations.

Under these conditions, parametric models of individual differences scaling, and more specifically, covariance structures models are superior to non parametric models. In particular, covariance structure models are clearly suited when it is of interest to model the relationships between a set of stimuli and some external variables.

**AUTHOR NOTES**

This research was made possible in part by Contracts No. N00014-89-K-059 and N0001490-J-1958 from the Office of Naval Technology, and by Office of Naval Research Contracts No. N00014-86K-0482, NR 442-1546, Michael Levine, principal investigator. The author's participation was supported by a Postdoctoral Scholarship from the Ministry of Education and Science of Spain (‘Beca Postdoctoral de Formación de Personal Investigador en el Extranjero'). The author is grateful to Michael Levine and especially to Ulf Böckenholt for their comments to a previous draft of this paper.

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*Aceptado el 27 de diciembre de 1993*