  In this catalog, we present the results of a systematic study of gamma-ray
bursts (GRBs) with reliable redshift estimates detected in the triggered mode
of the Konus-Wind (KW) experiment during the period from 1997 February to 2016
June. The sample consists of 150 GRBs (including twelve short/hard bursts) and
represents the largest set of cosmological GRBs studied to date over a broad
energy band. From the temporal and spectral analyses of the sample, we provide
the burst durations, the spectral lags, the results of spectral fits with two
model functions, the total energy fluences, and the peak energy fluxes. Based
on the GRB redshifts, which span the range 0.1 <= z <= 5, we estimate the
rest-frame, isotropic-equivalent energy and peak luminosity. For 32 GRBs with
reasonably-constrained jet breaks we provide the collimation-corrected values
of the energetics. We consider the behavior of the rest-frame GRB parameters in
the hardness-duration and hardness-intensity planes, and confirm the "Amati"
and "Yonetoku" relations for Type II GRBs. The correction for the jet
collimation does not improve these correlations for the KW sample. We discuss
the influence of instrumental selection effects on the GRB parameter
distributions and estimate the KW GRB detection horizon, which extends to z ~
16.6, stressing the importance of GRBs as probes of the early Universe.
Accounting for the instrumental bias, we estimate the KW GRB luminosity
evolution, luminosity and isotropic-energy functions, and the evolution of the
GRB formation rate, which are in general agreement with those obtained in
previous studies.
