  Studying the spatial distribution of extragalactic source populations is
vital in understanding the matter distribution in the Universe. It also enables
understanding the cosmological evolution of dark matter density fields and the
relationship between dark matter and luminous matter. Clustering studies are
also required for EoR foreground studies since it affects the relevant angular
scales. This paper investigates the angular and spatial clustering properties
and the bias parameter of radio-selected sources in the Lockman Hole field at
325 MHz. The data probes sources with fluxes $\gtrsim$0.3 mJy within a radius
of 1.8$^\circ$ around the phase center of a $6^\circ \times 6^\circ$ mosaic.
Based on their radio luminosity, the sources are classified into Active
Galactic Nuclei (AGNs) and Star-Forming Galaxies (SFGs). Clustering and bias
parameters are determined for the combined populations and the classified
sources. The spatial correlation length and the bias of AGNs are greater than
SFGs -- indicating that more massive haloes host the former. This study is the
first reported estimate of the clustering property of sources at 325 MHz,
intermediate between the preexisting studies at high and low-frequency bands.
It also probes a well-studied deep field at an unexplored frequency with
moderate depth and area. Clustering studies require such observations along
different lines of sight, with various fields and data sets across frequencies
to avoid cosmic variance and systematics. Thus, an extragalactic deep field has
been studied in this work to contribute to this knowledge.
