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

C. Gruppioni; P. Ciliegi; M. Rowan-Robinson; L. Cram; A. Hopkins; C. Cesarsky; L. Danese; A. Franceschini; R. Genzel; A. Lawrence; D. Lemke; R. G. McMahon; G. Miley; S. Oliver; J.-L. Puget; B. Rocca-Volmerange

doi:10.1046/j.1365-8711.1999.02415.x

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

C. Gruppioni, P. Ciliegi, M. Rowan-Robinson, L. Cram, A. Hopkins, C. Cesarsky, L. Danese, A. Franceschini, R. Genzel, A. Lawrence, D. Lemke, R. G. McMahon, G. Miley, S. Oliver, J.-L. Puget, B. Rocca-Volmerange

Research output: Contribution to journal › Article › peer-review

Abstract

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 deg^2, has also been surveyed in the mid- and far-infrared (5-200 μm) with the Infrared Space Observatory (ISO). The radio survey provides uniform coverage of the entire S1 region, with a sensitivity (5sigma) 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 5sigma 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

Original language	English
Pages (from-to)	297-308
Journal	Monthly Notices of the Royal Astronomical Society
Volume	305
Issue number	2
DOIs	https://doi.org/10.1046/j.1365-8711.1999.02415.x
Publication status	Published - 1 Apr 1999

Keywords / Materials (for Non-textual outputs)

SURVEYS
GALAXIES: STARBURST
COSMOLOGY: OBSERVATIONS
INFRARED: GALAXIES
RADIO CONTINUUM: GALAXIES

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10.1046/j.1365-8711.1999.02415.x

http://adsabs.harvard.edu/abs/1999MNRAS.305..297G

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Gruppioni, C., Ciliegi, P., Rowan-Robinson, M., Cram, L., Hopkins, A., Cesarsky, C., Danese, L., Franceschini, A., Genzel, R., Lawrence, A., Lemke, D., McMahon, R. G., Miley, G., Oliver, S., Puget, J.-L., & Rocca-Volmerange, B. (1999). A 1.4-GHz survey of the southern European Large-Area ISO Survey region. Monthly Notices of the Royal Astronomical Society, 305(2), 297-308. https://doi.org/10.1046/j.1365-8711.1999.02415.x

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title = "A 1.4-GHz survey of the southern European Large-Area ISO Survey region",

abstract = "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 deg\textasciicircum{}2, has also been surveyed in the mid- and far-infrared (5-200 μm) with the Infrared Space Observatory (ISO). The radio survey provides uniform coverage of the entire S1 region, with a sensitivity (5sigma) 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 5sigma 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",

keywords = "SURVEYS, GALAXIES: STARBURST, COSMOLOGY: OBSERVATIONS, INFRARED: GALAXIES, RADIO CONTINUUM: GALAXIES",

author = "C. Gruppioni and P. Ciliegi and M. Rowan-Robinson and L. Cram and A. Hopkins and C. Cesarsky and L. Danese and A. Franceschini and R. Genzel and A. Lawrence and D. Lemke and McMahon, \{R. G.\} and G. Miley and S. Oliver and J.-L. Puget and B. Rocca-Volmerange",

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doi = "10.1046/j.1365-8711.1999.02415.x",

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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, J-L & Rocca-Volmerange, B 1999, 'A 1.4-GHz survey of the southern European Large-Area ISO Survey region', Monthly Notices of the Royal Astronomical Society, vol. 305, no. 2, pp. 297-308. https://doi.org/10.1046/j.1365-8711.1999.02415.x

TY - JOUR

T1 - A 1.4-GHz survey of the southern European Large-Area ISO Survey 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 - 1999/4/1

Y1 - 1999/4/1

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 deg^2, has also been surveyed in the mid- and far-infrared (5-200 μm) with the Infrared Space Observatory (ISO). The radio survey provides uniform coverage of the entire S1 region, with a sensitivity (5sigma) 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 5sigma 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

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 deg^2, has also been surveyed in the mid- and far-infrared (5-200 μm) with the Infrared Space Observatory (ISO). The radio survey provides uniform coverage of the entire S1 region, with a sensitivity (5sigma) 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 5sigma 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

KW - SURVEYS

KW - GALAXIES: STARBURST

KW - COSMOLOGY: OBSERVATIONS

KW - INFRARED: GALAXIES

KW - RADIO CONTINUUM: GALAXIES

U2 - 10.1046/j.1365-8711.1999.02415.x

DO - 10.1046/j.1365-8711.1999.02415.x

M3 - Article

SN - 0035-8711

VL - 305

SP - 297

EP - 308

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 2

ER -

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

Abstract

Keywords / Materials (for Non-textual outputs)

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