  Three fields in the outskirts of the Small Magellanic Cloud were observed by
the Ultra-Violet Imaging Telescope (UVIT) on board AstroSat, during 31 December
2017 and 01 January 2018. The observations were carried out on a total of seven
filters, three in the far ultra-violet (FUV; 1300$-$1800 \r{A}) band and four
in the near ultra-violet (NUV; 2000$-$3000 \r{A}) band. We carried out
photometry of these observations that have a spatial resolution better than
1.5$^{\prime\prime}$. We present here the first results of this work, which is
a matched catalogue of 11,241 sources detected in three FUV and four NUV
wavelengths. We make the catalogue available online, which would be of use to
the astronomical community to address a wide variety of astrophysical problems.
We provide an expression to estimate the total count rate in the full point
spread function of UVIT that also incorporate the effect of saturation.
