A 1.4‐GHz survey of the southern European Large‐Area ISO Survey region
Identifieur interne : 00C551 ( Main/Exploration ); précédent : 00C550; suivant : 00C552A 1.4‐GHz survey of the southern European Large‐Area ISO Survey region
Auteurs : C. Gruppioni [Italie] ; P. Ciliegi [Italie] ; M. Rowan-Robinson ; L. Cram [Australie] ; A. Hopkins [Australie] ; C. Cesarsky [France] ; L. Danese [Italie] ; A. Franceschini [Italie] ; R. Genzel [Allemagne] ; A. Lawrence [Royaume-Uni] ; D. Lemke [Allemagne] ; R. G. Mcmahon ; G. Miley [Pays-Bas] ; S. Oliver ; J. Puget [France] ; B. Rocca-Volmerange [France]Source :
- Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 1999-04-24.
English descriptors
- KwdEn :
- Antenna gains, Arcmin, Arcsec, Areal coverage, Atca, Atca data, Atca survey, Australia telescope, Calibration errors, Calibrator, Centre, Ciliegi, Complementary samples, Complete sample, Condon, Continuum mode, Contour images, Crucial role, Deconvolution, Deg2, Density limit, Density ratios, Different surveys, Differential source counts, Elais, Eld, Full catalogue, Galaxy, Gaussian, Gruppioni, Infrared space observatory, Integral counts, Lled stars, Major axis, Mathis neuschaefer, Minor axes, Mnras, Mosaic, Mosaic errors, Mosaic technique, Multiple source, Multiple sources, Normal galaxies, Northern elais regions, Open circles, Optical phase, Osservatorio astronomico, Pixel, Pointings, Position angle, Position errors, Position uncertainties, Positional errors, Previous work, Primary beam, Primary calibrator, Radio counterparts, Radio observations, Radio sample, Radio source population, Radio sources, Right ascension, Same volume, Sault, Sault killeen, Secondary calibrator, Single pointings, Solid angle, Solid line, Solid lines, Source counts, Source extraction, Source parameters, Source position, Source size, Southern elais region, Spatial resolution, Star formation rate, Survey region, Total area, Total mosaic, Total source, Tting counts, Upper envelope, Weak sources, Whole area, Windhorst, cosmology: observations, galaxies: starburst, infrared: galaxies, radio continuum: galaxies, surveys.
- Teeft :
- Antenna gains, Arcmin, Arcsec, Areal coverage, Atca, Atca data, Atca survey, Australia telescope, Calibration errors, Calibrator, Centre, Ciliegi, Complementary samples, Complete sample, Condon, Continuum mode, Contour images, Crucial role, Deconvolution, Deg2, Density limit, Density ratios, Different surveys, Differential source counts, Elais, Eld, Full catalogue, Galaxy, Gaussian, Gruppioni, Infrared space observatory, Integral counts, Lled stars, Major axis, Mathis neuschaefer, Minor axes, Mnras, Mosaic, Mosaic errors, Mosaic technique, Multiple source, Multiple sources, Normal galaxies, Northern elais regions, Open circles, Optical phase, Osservatorio astronomico, Pixel, Pointings, Position angle, Position errors, Position uncertainties, Positional errors, Previous work, Primary beam, Primary calibrator, Radio counterparts, Radio observations, Radio sample, Radio source population, Radio sources, Right ascension, Same volume, Sault, Sault killeen, Secondary calibrator, Single pointings, Solid angle, Solid line, Solid lines, Source counts, Source extraction, Source parameters, Source position, Source size, Southern elais region, Spatial resolution, Star formation rate, Survey region, Total area, Total mosaic, Total source, Tting counts, Upper envelope, Weak sources, Whole area, Windhorst.
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 deg2, 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 (5σ) 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 5σ 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
Url:
- https://api.istex.fr/document/08A8907E054904F763AC29BD1C6D1AA2A038B92C/fulltext/pdf
- https://api.istex.fr/document/2E5B6436F177D16B254D30CE3E78BB6CC399AFB2/fulltext/pdf
DOI: 10.1046/j.1365-8711.1999.02415.x
Affiliations:
- Allemagne, Australie, France, Italie, Pays-Bas, Royaume-Uni
- Bade-Wurtemberg, District de Karlsruhe, Hollande-Méridionale, Nouvelle-Galles du Sud, Écosse, Île-de-France
- Gif‐sur‐Yvette, Heidelberg, Leyde, Orsay, Sydney, Édimbourg
- Université Paris-Sud, Université d'Édimbourg, Université de Sydney
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- to stream Istex, to step Curation: 000898
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- to stream Main, to step Curation: 00C551
Le document en format XML
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Gruppioni</name><affiliation></affiliation><affiliation wicri:level="1"><country xml:lang="fr">Italie</country><wicri:regionArea>Osservatorio Astronomico di Bologna, via Ranzani 1, Bologna</wicri:regionArea><wicri:noRegion>Bologna</wicri:noRegion></affiliation></author><author><name sortKey="Ciliegi, P" sort="Ciliegi, P" uniqKey="Ciliegi P" first="P." last="Ciliegi">P. Ciliegi</name><affiliation wicri:level="1"><country xml:lang="fr">Italie</country><wicri:regionArea>Osservatorio Astronomico di Bologna, via Ranzani 1, Bologna</wicri:regionArea><wicri:noRegion>Bologna</wicri:noRegion></affiliation><affiliation></affiliation></author><author><name sortKey="Rowan Obinson, M" sort="Rowan Obinson, M" uniqKey="Rowan Obinson M" first="M." last="Rowan-Robinson">M. Rowan-Robinson</name><affiliation><wicri:noCountry code="subField">2BZ</wicri:noCountry></affiliation></author><author><name sortKey="Cram, L" sort="Cram, L" uniqKey="Cram L" first="L." last="Cram">L. 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Franceschini</name><affiliation wicri:level="1"><country xml:lang="fr">Italie</country><wicri:regionArea>Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, I‐‐35122 Padova</wicri:regionArea><wicri:noRegion>I‐‐35122 Padova</wicri:noRegion></affiliation></author><author><name sortKey="Genzel, R" sort="Genzel, R" uniqKey="Genzel R" first="R." last="Genzel">R. Genzel</name><affiliation wicri:level="1"><country xml:lang="fr">Allemagne</country><wicri:regionArea>Max‐Planck‐Institut für Extraterrestrische Physik, Giessenbachstrasse, D‐8046 Garching bei München</wicri:regionArea><wicri:noRegion>D‐8046 Garching bei München</wicri:noRegion><wicri:noRegion>D‐8046 Garching bei München</wicri:noRegion></affiliation></author><author><name sortKey="Lawrence, A" sort="Lawrence, A" uniqKey="Lawrence A" first="A." last="Lawrence">A. Lawrence</name><affiliation wicri:level="4"><orgName type="university">Université d'Édimbourg</orgName><country>Royaume-Uni</country><placeName><settlement type="city">Édimbourg</settlement><region type="country">Écosse</region></placeName></affiliation></author><author><name sortKey="Lemke, D" sort="Lemke, D" uniqKey="Lemke D" first="D." last="Lemke">D. Lemke</name><affiliation wicri:level="3"><country xml:lang="fr">Allemagne</country><wicri:regionArea>Max‐Planck Institute, Heidelberg</wicri:regionArea><placeName><region type="land" nuts="1">Bade-Wurtemberg</region><region type="district" nuts="2">District de Karlsruhe</region><settlement type="city">Heidelberg</settlement></placeName></affiliation></author><author><name sortKey="Mcmahon, R G" sort="Mcmahon, R G" uniqKey="Mcmahon R" first="R. G." last="Mcmahon">R. G. Mcmahon</name><affiliation><wicri:noCountry code="subField">0HA</wicri:noCountry></affiliation></author><author><name sortKey="Miley, G" sort="Miley, G" uniqKey="Miley G" first="G." last="Miley">G. Miley</name><affiliation wicri:level="3"><country xml:lang="fr" wicri:curation="lc">Pays-Bas</country><wicri:regionArea>Leiden Observatory, PO Box 9513, 2300 RA, Leiden</wicri:regionArea><placeName><settlement type="city">Leyde</settlement><region nuts="2" type="province">Hollande-Méridionale</region></placeName></affiliation></author><author><name sortKey="Oliver, S" sort="Oliver, S" uniqKey="Oliver S" first="S." last="Oliver">S. Oliver</name><affiliation><wicri:noCountry code="subField">2BZ</wicri:noCountry></affiliation></author><author><name sortKey="Puget, J" sort="Puget, J" uniqKey="Puget J" first="J." last="Puget">J. Puget</name><affiliation wicri:level="4"><country xml:lang="fr">France</country><wicri:regionArea>Institut d'Astrophysique Spatiale, Bat. 121, Université Paris XI, F‐91405 Orsay Cedex</wicri:regionArea><orgName type="university">Université Paris-Sud</orgName><placeName><settlement type="city">Orsay</settlement><region type="region" nuts="2">Île-de-France</region></placeName></affiliation></author><author><name sortKey="Rocca Olmerange, B" sort="Rocca Olmerange, B" uniqKey="Rocca Olmerange B" first="B." last="Rocca-Volmerange">B. Rocca-Volmerange</name><affiliation wicri:level="4"><country xml:lang="fr">France</country><wicri:regionArea>Institut d'Astrophysique Spatiale, Bat. 121, Université Paris XI, F‐91405 Orsay Cedex</wicri:regionArea><orgName type="university">Université Paris-Sud</orgName><placeName><settlement type="city">Orsay</settlement><region type="region" nuts="2">Île-de-France</region></placeName></affiliation><affiliation wicri:level="1"><country xml:lang="fr">France</country><wicri:regionArea>Institut d'Astrophysique de Paris, CNRS, 98 bis Bd. Arago, F‐75014 Paris</wicri:regionArea><wicri:noRegion>75014 Paris</wicri:noRegion><wicri:noRegion>F‐75014 Paris</wicri:noRegion></affiliation></author></analytic><monogr></monogr><series><title level="j" type="main">Monthly Notices of the Royal Astronomical Society</title><title level="j" type="alt">MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY</title><idno type="ISSN">0035-8711</idno><idno type="eISSN">1365-2966</idno><imprint><biblScope unit="vol">305</biblScope><biblScope unit="issue">2</biblScope><biblScope unit="page" from="297">297</biblScope><biblScope unit="page" to="308">308</biblScope><biblScope unit="page-count">12</biblScope><publisher>Blackwell Science Ltd.</publisher><pubPlace>Oxford, UK</pubPlace><date type="published" when="1999-04-24">1999-04-24</date></imprint><idno type="ISSN">0035-8711</idno></series></biblStruct></sourceDesc><seriesStmt><idno type="ISSN">0035-8711</idno></seriesStmt></fileDesc><profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>Antenna gains</term><term>Arcmin</term><term>Arcsec</term><term>Areal coverage</term><term>Atca</term><term>Atca data</term><term>Atca survey</term><term>Australia telescope</term><term>Calibration errors</term><term>Calibrator</term><term>Centre</term><term>Ciliegi</term><term>Complementary samples</term><term>Complete sample</term><term>Condon</term><term>Continuum mode</term><term>Contour images</term><term>Crucial role</term><term>Deconvolution</term><term>Deg2</term><term>Density limit</term><term>Density ratios</term><term>Different surveys</term><term>Differential source counts</term><term>Elais</term><term>Eld</term><term>Full catalogue</term><term>Galaxy</term><term>Gaussian</term><term>Gruppioni</term><term>Infrared space observatory</term><term>Integral counts</term><term>Lled stars</term><term>Major axis</term><term>Mathis neuschaefer</term><term>Minor axes</term><term>Mnras</term><term>Mosaic</term><term>Mosaic errors</term><term>Mosaic technique</term><term>Multiple source</term><term>Multiple sources</term><term>Normal galaxies</term><term>Northern elais regions</term><term>Open circles</term><term>Optical phase</term><term>Osservatorio astronomico</term><term>Pixel</term><term>Pointings</term><term>Position angle</term><term>Position errors</term><term>Position uncertainties</term><term>Positional errors</term><term>Previous work</term><term>Primary beam</term><term>Primary calibrator</term><term>Radio counterparts</term><term>Radio observations</term><term>Radio sample</term><term>Radio source population</term><term>Radio sources</term><term>Right ascension</term><term>Same volume</term><term>Sault</term><term>Sault killeen</term><term>Secondary calibrator</term><term>Single pointings</term><term>Solid angle</term><term>Solid line</term><term>Solid lines</term><term>Source counts</term><term>Source extraction</term><term>Source parameters</term><term>Source position</term><term>Source size</term><term>Southern elais region</term><term>Spatial resolution</term><term>Star formation rate</term><term>Survey region</term><term>Total area</term><term>Total mosaic</term><term>Total source</term><term>Tting counts</term><term>Upper envelope</term><term>Weak sources</term><term>Whole area</term><term>Windhorst</term><term>cosmology: observations</term><term>galaxies: starburst</term><term>infrared: galaxies</term><term>radio continuum: galaxies</term><term>surveys</term></keywords><keywords scheme="Teeft" xml:lang="en"><term>Antenna gains</term><term>Arcmin</term><term>Arcsec</term><term>Areal coverage</term><term>Atca</term><term>Atca data</term><term>Atca survey</term><term>Australia telescope</term><term>Calibration errors</term><term>Calibrator</term><term>Centre</term><term>Ciliegi</term><term>Complementary samples</term><term>Complete sample</term><term>Condon</term><term>Continuum mode</term><term>Contour images</term><term>Crucial role</term><term>Deconvolution</term><term>Deg2</term><term>Density limit</term><term>Density ratios</term><term>Different surveys</term><term>Differential source counts</term><term>Elais</term><term>Eld</term><term>Full catalogue</term><term>Galaxy</term><term>Gaussian</term><term>Gruppioni</term><term>Infrared space observatory</term><term>Integral counts</term><term>Lled stars</term><term>Major axis</term><term>Mathis neuschaefer</term><term>Minor axes</term><term>Mnras</term><term>Mosaic</term><term>Mosaic errors</term><term>Mosaic technique</term><term>Multiple source</term><term>Multiple sources</term><term>Normal galaxies</term><term>Northern elais regions</term><term>Open circles</term><term>Optical phase</term><term>Osservatorio astronomico</term><term>Pixel</term><term>Pointings</term><term>Position angle</term><term>Position errors</term><term>Position uncertainties</term><term>Positional errors</term><term>Previous work</term><term>Primary beam</term><term>Primary calibrator</term><term>Radio counterparts</term><term>Radio observations</term><term>Radio sample</term><term>Radio source population</term><term>Radio sources</term><term>Right ascension</term><term>Same volume</term><term>Sault</term><term>Sault killeen</term><term>Secondary calibrator</term><term>Single pointings</term><term>Solid angle</term><term>Solid line</term><term>Solid lines</term><term>Source counts</term><term>Source extraction</term><term>Source parameters</term><term>Source position</term><term>Source size</term><term>Southern elais region</term><term>Spatial resolution</term><term>Star formation rate</term><term>Survey region</term><term>Total area</term><term>Total mosaic</term><term>Total source</term><term>Tting counts</term><term>Upper envelope</term><term>Weak sources</term><term>Whole area</term><term>Windhorst</term></keywords></textClass></profileDesc></teiHeader><front><div type="abstract" xml:lang="en">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 deg2, 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 (5σ) 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 5σ 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</div></front></TEI><affiliations><list><country><li>Allemagne</li><li>Australie</li><li>France</li><li>Italie</li><li>Pays-Bas</li><li>Royaume-Uni</li></country><region><li>Bade-Wurtemberg</li><li>District de Karlsruhe</li><li>Hollande-Méridionale</li><li>Nouvelle-Galles du Sud</li><li>Écosse</li><li>Île-de-France</li></region><settlement><li>Gif‐sur‐Yvette</li><li>Heidelberg</li><li>Leyde</li><li>Orsay</li><li>Sydney</li><li>Édimbourg</li></settlement><orgName><li>Université Paris-Sud</li><li>Université d'Édimbourg</li><li>Université de Sydney</li></orgName></list><tree><noCountry><name sortKey="Mcmahon, R G" sort="Mcmahon, R G" uniqKey="Mcmahon R" first="R. G." last="Mcmahon">R. G. Mcmahon</name><name sortKey="Oliver, S" sort="Oliver, S" uniqKey="Oliver S" first="S." last="Oliver">S. Oliver</name><name sortKey="Rowan Obinson, M" sort="Rowan Obinson, M" uniqKey="Rowan Obinson M" first="M." last="Rowan-Robinson">M. Rowan-Robinson</name></noCountry><country name="Italie"><noRegion><name sortKey="Gruppioni, C" sort="Gruppioni, C" uniqKey="Gruppioni C" first="C." last="Gruppioni">C. Gruppioni</name></noRegion><name sortKey="Ciliegi, P" sort="Ciliegi, P" uniqKey="Ciliegi P" first="P." last="Ciliegi">P. Ciliegi</name><name sortKey="Danese, L" sort="Danese, L" uniqKey="Danese L" first="L." last="Danese">L. Danese</name><name sortKey="Franceschini, A" sort="Franceschini, A" uniqKey="Franceschini A" first="A." last="Franceschini">A. Franceschini</name></country><country name="Australie"><region name="Nouvelle-Galles du Sud"><name sortKey="Cram, L" sort="Cram, L" uniqKey="Cram L" first="L." last="Cram">L. Cram</name></region><name sortKey="Hopkins, A" sort="Hopkins, A" uniqKey="Hopkins A" first="A." last="Hopkins">A. Hopkins</name></country><country name="France"><region name="Île-de-France"><name sortKey="Cesarsky, C" sort="Cesarsky, C" uniqKey="Cesarsky C" first="C." last="Cesarsky">C. Cesarsky</name></region><name sortKey="Puget, J" sort="Puget, J" uniqKey="Puget J" first="J." last="Puget">J. Puget</name><name sortKey="Rocca Olmerange, B" sort="Rocca Olmerange, B" uniqKey="Rocca Olmerange B" first="B." last="Rocca-Volmerange">B. Rocca-Volmerange</name><name sortKey="Rocca Olmerange, B" sort="Rocca Olmerange, B" uniqKey="Rocca Olmerange B" first="B." last="Rocca-Volmerange">B. Rocca-Volmerange</name></country><country name="Allemagne"><noRegion><name sortKey="Genzel, R" sort="Genzel, R" uniqKey="Genzel R" first="R." last="Genzel">R. Genzel</name></noRegion><name sortKey="Lemke, D" sort="Lemke, D" uniqKey="Lemke D" first="D." last="Lemke">D. Lemke</name></country><country name="Royaume-Uni"><region name="Écosse"><name sortKey="Lawrence, A" sort="Lawrence, A" uniqKey="Lawrence A" first="A." last="Lawrence">A. Lawrence</name></region></country><country name="Pays-Bas"><region name="Hollande-Méridionale"><name sortKey="Miley, G" sort="Miley, G" uniqKey="Miley G" first="G." last="Miley">G. Miley</name></region></country></tree></affiliations></record>Pour manipuler ce document sous Unix (Dilib)
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|area= AustralieFrV1
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|texte= A 1.4‐GHz survey of the southern European Large‐Area ISO Survey region
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