A deep survey of the European Large-Area ISO Survey (ELAIS) field in the so
uthern celestial hemisphere thereinafter Sl)has been carried out with the A
ustralia Telescope Compact Array (ATCA) at 1.4 GHz. The S1 region, covering
about 4 deg(2), has also been surveyed in the mid-and far-infrared (5-200
mu m) with the Infrared Space Observatory (ISO). The radio survey provides
uniform coverage of the entire SI region, with a sensitivity (5 sigma) of 0
.4 mJy over the whole area and 0.2 mJy in the centre. To this sensitivity,
virtually all the radio counterparts of the far-infrared extragalactic ISO
sources should be detected. This paper presents a radio sample - complete a
t the 5 sigma level - consisting of 581 sources detected at 1.4 GHz. Of the
se radio sources, 349 have peak flux density in the range 0.2-1 mJy, formin
g a new homogeneous sample of sub-mJy radio sources. Due to its size, depth
and multiwaveband coverage, the sample will allow us to study in greater d
etail the sub-mJy radio source population. The full catalogue will be avail
able from http://athena.ph.ic.ac.uk/pubs.html.