If the Hessian is available, summary.hyperbFit computes
standard errors for the estimates of \(\pi\), \(\zeta\),
\(\delta\), and \(\mu\), and adds them to object
as object$sds. Otherwise, no calculations are performed and the
composition of object is unaltered.
summary.hyperbFit invisibly returns x
with class changed to summary.hyperbFit.
See hyperbFit for the composition of an object of class
hyperbFit.
print.summary.hyperbFit prints a summary in the same format as
print.hyperbFit when the Hessian is not available from
the fit. When the Hessian is available, the standard errors for the
parameter estimates are printed in parentheses beneath the parameter
estimates, in the manner of fitdistr in the package
MASS.