  $\require{mediawiki-texvc}$ Supermassive black holes at the centre of active
galactic nuclei (AGN) produce relativistic jets that can affect the star
formation characteristics of the AGN hosts. Observations in the ultraviolet
(UV) band can provide an excellent view of the effect of AGN jets on star
formation. Here, we present a census of star formation properties in the
Northern Star-forming Region (NSR) that spans about 20 kpc of the large radio
source Centaurus A hosted by the giant elliptical galaxy NGC 5128. In this
region, we identified 352 UV sources associated with Cen A using new
observations at an angular resolution of $<$1.5 arcseconds observed with the
Ultra-Violet Imaging Telescope (UVIT) onboard AstroSat. These observations were
carried out in one far-ultraviolet (FUV; $\lambda_{\text{mean}}$ = 1481 $\AA$)
and three near-ultraviolet (NUV; with $\lambda_{\text{mean}}$ of 2196 $\AA$,
2447 $\AA$, and 2792 $\AA$, respectively) bands. The star-forming sources
identified in UV tend to lie in the direction of the jet of Cen A, thereby
suggesting jet triggering of star formation. Separating the NSR into Outer and
Inner regions, we found the stars in the Inner region to have a relatively
younger age than the Outer region, suggesting that the two regions may have
different star formation histories. We also provide the UVIT source catalogue
in the NSR.
