  Data from the Gaia satellite are revolutionising our understanding of the
Milky Way. With every new data release, there is a need to update the census of
open clusters. We aim to conduct a blind, all-sky search for open clusters
using 729 million sources from Gaia DR3 down to magnitude $G\sim20$, creating a
homogeneous catalogue of clusters including many new objects. We used the
Hierarchical Density-Based Spatial Clustering of Applications with Noise
(HDBSCAN) algorithm to recover clusters. We validated our clusters using a
statistical density test and a Bayesian convolutional neural network for
colour-magnitude diagram classification. We inferred basic astrometric
parameters, ages, extinctions, and distances for the clusters in the catalogue.
We recovered 7167 clusters, 2387 of which are candidate new objects and 4782 of
which crossmatch to objects in the literature, including 134 globular clusters.
A more stringent cut of our catalogue contains 4105 highly reliable clusters,
739 of which are new. Owing to the scope of our methodology, we are able to
tentatively suggest that many of the clusters we are unable to detect may not
be real, including 1152 clusters from the Milky Way Star Cluster (MWSC)
catalogue that should have been detectable in Gaia data. Our cluster membership
lists include many new members and often include tidal tails. Our catalogue's
distribution traces the galactic warp, the spiral arm structure, and the dust
distribution of the Milky Way. While much of the content of our catalogue
contains bound open and globular clusters, as many as a few thousand of our
clusters are more compatible with unbound moving groups, which we will classify
in an upcoming work. We have conducted the largest search for open clusters to
date, producing a single homogeneous star cluster catalogue which we make
available with this paper.
