  Despite having data for over 10^9 stars from Gaia, only less than 10^4 star
clusters and candidates have been discovered. Particularly, distant star
clusters are rarely identified, due to the challenges posed by heavy extinction
and great distance. However, Gaia data has continued to improve, enabling even
fainter cluster members to be distinguished from field stars. In this work, we
will introduce a star cluster search method based on the DBSCAN algorithm; we
have made improvements to make it better suited for identifying clusters on
dimmer and more distant stars. After removing member stars of known Gaia-based
clusters, we have identified 2086 objects with |b|<10 deg, of which 1488 are
highly reliable open star clusters, along with 569 candidates, 28 globular
cluster candidates and 1 irregular galaxy IC 10 at low Galactic latitudes. We
found that the proper motion of IC10 is similar yet slightly different from the
water maser observations, which is an important result for the comparison with
Gaia and VLBA. Besides, when compared with the star clusters appearing in Gaia
DR2/EDR3, we have found nearly three times as many new objects above a distance
of 5 kpc, including hundreds of them above Av > 5 mag. And it has enabled us to
detect a higher number of old clusters, over a billion years old, that are
difficult to detect due to observational limitations. Our findings
significantly expand the remote cluster sample and enhance our understanding of
the limits of Gaia DR3 data in stellar aggregates research. The full figure set
for 2085 clusters can be seen in \url{https://nadc.china-vo.org/res/r101258/}

Astrophysics of Galaxies