  We show that each of the three Dainotti-correlated gamma-ray burst (GRB) data
sets recently compiled by Wang et al. and Hu et al., that together probe the
redshift range $0.35 \leq z \leq 5.91$, obey cosmological-model-independent
Dainotti correlation relations and so are standardizable. We use these GRB data
in conjunction with the best currently-available Amati-correlated GRB data,
that probe $0.3399 \leq z \leq 8.2$, to constrain cosmological model
parameters. The resulting cosmological constraints are weak, providing lower
limits on the non-relativistic matter density parameter, mildly favoring
non-zero spatial curvature, and largely consistent with currently accelerated
cosmological expansion as well as with constraints determined from
better-established data.
