  Galaxy clusters are an essential tool to understand and constrain the
cosmological parameters of our Universe. Thanks to its multi-band design, J-PAS
offers a unique group and cluster detection window using precise photometric
redshifts and sufficient depths. We produce galaxy cluster catalogues from the
miniJPAS, which is a pathfinder survey for the wider J-PAS survey, using the
PZWav algorithm. Relying only on photometric information, we provide optical
mass tracers for the identified clusters, including richness, optical
luminosity, and stellar mass. By reanalysing the Chandra mosaic of the AEGIS
field, alongside the overlapping XMM-Newton observations, we produce an X-ray
catalogue. The analysis reveals the possible presence of structures with masses
of 4$\times 10^{13}$ M$_\odot$ at redshift 0.75, highlighting the depth of the
survey. Comparing results with those from two other cluster catalogues,
provided by AMICO and VT, we find $43$ common clusters with cluster centre
offsets of 100$\pm$60 kpc and redshift differences below 0.001. We provide a
comparison of the cluster catalogues with a catalogue of massive galaxies and
report on the significance of cluster selection. In general, we are able to
recover approximately 75$\%$ of the galaxies with $M^{\star} >$2$\times
10^{11}$ M$_\odot$. This study emphasises the potential of the J-PAS survey and
the employed techniques down to the group scales.
