accuracy | R Documentation |
Produces a table of fit statistics for multiple models.
accuracy(fits, plotit = FALSE, digits = 3, ...)
fits |
A series of model object names. Must be a list of model objects or a single model object. |
plotit |
If |
digits |
The number of significant digits in the output. |
... |
Other arguments passed to |
Produces a table of fit statistics for multiple models: minimum maximum accuracy, mean absolute percentage error, median absolute error, root mean square error, normalized root mean square error, Efron's pseudo r-squared, and coefficient of variation.
For minimum maximum accuracy, larger indicates a better fit, and a perfect fit is equal to 1.
For mean absolute error (MAE), smaller
indicates a better fit,
and a perfect fit is equal to 0.
It has the same units as the dependent variable.
Note that here, MAE is simply the mean of the absolute
values of the differences of predicted values and the
observed values
(MAE = mean(abs(predy - actual))
).
There are other definitions of MAE and similar-sounding
terms.
Median absolute error (MedAE) is similar, except employing the median rather than the mean.
For mean absolute percent error (MAPE), smaller indicates a better fit, and a perfect fit is equal to 0. The result is reported as a fraction. That is, a result of 0.1 is equal to 10 percent.
Root mean square error (RMSE) has the same units as the predicted values.
Normalized root mean square error (NRMSE) is RMSE divided by the mean or the median of the values of the dependent variable.
Efron's pseudo r-squared is calculated as 1 minus the residual sum
of squares divided by the total sum of squares. For linear models
(lm
model objects), Efron's pseudo r-squared will be equal
to r-squared. For other models, it should not be interpreted
as r-squared, but can still be useful as a relative measure.
CV.prcnt
is the coefficient of variation for the model.
Here it is expressed as a percent. That is, a result of 10 =
10 percent.
Model objects currently supported: lm, glm, nls, betareg, gls, lme, lmer, lmerTest, glmmTMB, rq, loess, gam, glm.nb, glmRob, mblm, and rlm.
A list of two objects: The series of model calls, and a data frame of statistics for each model.
Salvatore Mangiafico, mangiafico@njaes.rutgers.edu
https://rcompanion.org/handbook/G_14.html
compareLM
,
compareGLM
,
nagelkerke
data(BrendonSmall)
BrendonSmall$Calories = as.numeric(BrendonSmall$Calories)
BrendonSmall$Calories2 = BrendonSmall$Calories ^ 2
model.1 = lm(Sodium ~ Calories, data = BrendonSmall)
accuracy(model.1, plotit=FALSE)
model.2 = lm(Sodium ~ Calories + Calories2, data = BrendonSmall)
model.3 = glm(Sodium ~ Calories, data = BrendonSmall, family="Gamma")
quadplat = function(x, a, b, clx) {
ifelse(x < clx, a + b * x + (-0.5*b/clx) * x * x,
a + b * clx + (-0.5*b/clx) * clx * clx)}
model.4 = nls(Sodium ~ quadplat(Calories, a, b, clx),
data = BrendonSmall,
start = list(a=519, b=0.359, clx = 2300))
accuracy(list(model.1, model.2, model.3, model.4), plotit=FALSE)
### Perfect and poor model fits
X = c(1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12)
Y = c(1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12)
Z = c(1, 12, 13, 6, 10, 13, 4, 3, 5, 6, 10, 14)
perfect = lm(Y ~ X)
poor = lm(Z ~ X)
accuracy(list(perfect, poor), plotit=FALSE)
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