The methods documented on this page are actually some of the least important methods defined for sstapreg objects. The most important methods are documented separately, each with its own page. Links to those pages are provided in the See Also section, below.
# S3 method for sstapreg coef(object, ...) # S3 method for sstapreg confint(object, ...) # S3 method for sstapreg fitted(object, ...) # S3 method for sstapreg se(object, ...) # S3 method for sstapreg nobs(object, ...) # S3 method for sstapreg VarCorr(x) # S3 method for sstapreg ngrps(object, ...) # S3 method for sstapreg vcov(object, correlation = FALSE, ...) # S3 method for sstapreg nsamples(object, ...)
| object | sstapreg object |
|---|---|
| ... | Ignored |
| x | sstapreg object |
| correlation | For |
The methods documented on this page are similar to the methods defined for objects of class 'lm', 'glm', 'glmer', etc. However there are a few key differences:
coefMedians are used for fixed effect point estimates. See the Point estimates section
in print.sstapreg for more details.
seThe se function returns fixed effects standard errors based on
mad. See the Uncertainty estimates section in
print.sstapreg for more details.
confintconfint will throw an error because the
posterior_interval function should be used to compute Bayesian
uncertainty intervals.