  The Fourth Open Gravitational-wave Catalogue (4-OGC) presented parameter
estimation analyses for a number of gravitational wave triggers which had not
previously been presented in catalogues published by the LIGO, Virgo, and KAGRA
Collaborations (LVK). In this paper we present an analysis of these new
triggers using the same analysis workflow which was used to generate the
GWTC-2.1 and GWTC-3 catalogues published by the LVK, using a comparable
analysis configuration. We do not find any significant differences between our
analysis and that previously presented by 4-OGC, providing a reassuring
cross-check between two differing analysis techniques. We provide our parameter
estimation results in a format comparable to those of the GWTC-3 data release.
