TY - UNPB
T1 - A 1.4 GHz Survey of the Southern ELAIS Region
AU - Gruppioni, C.
AU - Ciliegi, P.
AU - Rowan-Robinson, M.
AU - Cram, L.
AU - Hopkins, A.
AU - Cesarsky, C.
AU - Danese, L.
AU - Franceschini, A.
AU - Genzel, R.
AU - Lawrence, A.
AU - Lemke, D.
AU - McMahon, R. G.
AU - Miley, G.
AU - Oliver, S.
AU - Puget, J-L.
AU - Rocca-Volmerange, B.
PY - 1998/12/1
Y1 - 1998/12/1
N2 - A deep survey of the European Large Area ISO Survey (ELAIS) field in the
southern celestial hemisphere (hereinafter S1) has been carried out with
the Australia Telescope Compact Array (ATCA) at 1.4 GHz. The S1 region,
covering about 4 square degrees, has been also surveyed in the mid- and
far-infrared (5-200 micron) with the Infrared Space Observatory (ISO).
The radio survey provides uniform coverage of the entire S1 region, with
a sensitivity (5 sigma) of 0.4 mJy over the whole area and 0.2 mJy in
the center. 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 at the 5 sigma level -
consisting of 581 sources detected at 1.4 GHz. Of these radio sources,
349 have peak flux density in the range 0.2-1 mJy, forming a new
homogeneous sample of sub-mJy radio sources. Due to its size, depth and
multi-waveband coverage, the sample will allow us to study in greater
detail the sub-mJy radio source population. The full catalogue will be
available from http://athena.ph.ac.uk/
AB - A deep survey of the European Large Area ISO Survey (ELAIS) field in the
southern celestial hemisphere (hereinafter S1) has been carried out with
the Australia Telescope Compact Array (ATCA) at 1.4 GHz. The S1 region,
covering about 4 square degrees, has been also surveyed in the mid- and
far-infrared (5-200 micron) with the Infrared Space Observatory (ISO).
The radio survey provides uniform coverage of the entire S1 region, with
a sensitivity (5 sigma) of 0.4 mJy over the whole area and 0.2 mJy in
the center. 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 at the 5 sigma level -
consisting of 581 sources detected at 1.4 GHz. Of these radio sources,
349 have peak flux density in the range 0.2-1 mJy, forming a new
homogeneous sample of sub-mJy radio sources. Due to its size, depth and
multi-waveband coverage, the sample will allow us to study in greater
detail the sub-mJy radio source population. The full catalogue will be
available from http://athena.ph.ac.uk/
KW - Astrophysics
M3 - Working paper
SP - 12256
BT - A 1.4 GHz Survey of the Southern ELAIS Region
PB - ArXiv
ER -