A 1.4-GHz survey of the southern European Large-Area ISO Survey region

被引:64
作者
Gruppioni, C
Ciliegi, P
Rowan-Robinson, M
Cram, L
Hopkins, A
Cesarsky, C
Danese, L
Franceschini, A
Genzel, R
Lawrence, A
Lemke, D
McMahon, RG
Miley, G
Oliver, S
Puget, JL
Rocca-Volmerange, B
机构
[1] Imperial Coll, Astrophys Grp, London SW7 2BZ, England
[2] Osservatorio Astron Bologna, I-40127 Bologna, Italy
[3] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England
[4] Univ Sydney, Sch Phys, Sydney, NSW 2006, Australia
[5] CENS, Serv Astrophys, F-91191 Gif Sur Yvette, France
[6] SISSA, I-34014 Trieste, Italy
[7] Osserv Astron Padova, I-35122 Padua, Italy
[8] Max Planck Inst Extraterr Phys, D-37075 Garching, Germany
[9] Univ Edinburgh, Inst Astron, Edinburgh EH9 3HJ, Midlothian, Scotland
[10] Max Planck Inst, Heidelberg, Germany
[11] Leiden Observ, NL-2300 RA Leiden, Netherlands
[12] Univ Paris 11, Inst Astrophys Spatiale, F-91405 Orsay, France
[13] CNRS, Inst Astrophys, F-75014 Paris, France
关键词
surveys; galaxies : starburst; cosmology : observations; infrared : galaxies; radio continuum : galaxies;
D O I
10.1046/j.1365-8711.1999.02415.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A deep survey of the European Large-Area ISO Survey (ELAIS) field in the southern celestial hemisphere thereinafter Sl)has been carried out with the Australia 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 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 multiwaveband 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.ic.ac.uk/pubs.html.
引用
收藏
页码:297 / 308
页数:12
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