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Studying the spatial distribution of extragalactic source populations isvital in understanding the matter distribution in the Universe. It also enablesunderstanding the cosmological evolution of dark matter density fields and therelationship between dark matter and luminous matter. Clustering studies arealso required for EoR foreground studies since it affects the relevant angularscales. This paper investigates the angular and spatial clustering propertiesand the bias parameter of radio-selected sources in the Lockman Hole field at325 MHz. The data probes sources with fluxes $\gtrsim$0.3 mJy within a radiusof 1.8$^\circ$ around the phase center of a $6^\circ \times 6^\circ$ mosaic.Based on their radio luminosity, the sources are classified into ActiveGalactic Nuclei (AGNs) and Star-Forming Galaxies (SFGs). Clustering and biasparameters are determined for the combined populations and the classifiedsources. The spatial correlation length and the bias of AGNs are greater thanSFGs -- indicating that more massive haloes host the former. This study is thefirst 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 withmoderate depth and area. Clustering studies require such observations alongdifferent lines of sight, with various fields and data sets across frequenciesto avoid cosmic variance and systematics. Thus, an extragalactic deep field hasbeen studied in this work to contribute to this knowledge.

A study on the Clustering Properties of Radio-Selected sources in the Lockman Hole Region at 325 MHz