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The XMM-Newton serendipitous survey. IV. Optical identification of the XMM-Newton medium sensitivity survey (XMS)

Identifieur interne : 009311 ( Main/Exploration ); précédent : 009310; suivant : 009312

The XMM-Newton serendipitous survey. IV. Optical identification of the XMM-Newton medium sensitivity survey (XMS)

Auteurs : X. Barcons [Espagne] ; F. J. Carrera [Espagne] ; M. T. Ceballos [Espagne] ; M. J. Page [Royaume-Uni] ; J. Bussons-Gordo [Espagne] ; A. Corral [Espagne] ; J. Ebrero [Espagne] ; S. Mateos [Espagne, Royaume-Uni] ; J. A. Tedds [Royaume-Uni] ; M. G. Watson [Royaume-Uni] ; D. Baskill [Royaume-Uni] ; M. Birkinshaw [Royaume-Uni] ; T. Boller [Allemagne] ; N. Borisov [Russie] ; M. Bremer [Royaume-Uni] ; G. E. Bromage [Royaume-Uni] ; H. Brunner [Allemagne] ; A. Caccianiga [Italie] ; C. S. Crawford [Royaume-Uni] ; M. S. Cropper [Royaume-Uni] ; R. Della Ceca [Italie] ; P. Derry [Royaume-Uni] ; A. C. Fabian [Royaume-Uni] ; P. Guillout [France] ; Y. Hashimoto [Allemagne] ; G. Hasinger [Allemagne] ; B. J. M. Hassall [Royaume-Uni] ; G. Lamer [Allemagne] ; N. S. Loaring [Royaume-Uni, Afrique du Sud] ; T. Maccacaro [Italie] ; K. O. Mason [Royaume-Uni] ; R. G. Mcmahon [Royaume-Uni] ; L. Mirioni [France] ; J. P. D. Mittaz [Royaume-Uni] ; C. Motch [France] ; I. Negueruela [France, Espagne] ; J. P. Osborne [Royaume-Uni] ; F. Panessa [Espagne] ; I. Perez-Foumon [Espagne] ; J. P. Pye [Royaume-Uni] ; T. P. Roberts [Royaume-Uni] ; S. Rosen [Royaume-Uni] ; N. Schartel [Espagne] ; N. Schurch [Royaume-Uni] ; A. Schwope [Allemagne] ; P. Severgnin [Espagne] ; R. Sharp [Royaume-Uni, Australie] ; G. C. Stewart [Royaume-Uni] ; G. Szokoly [Allemagne] ; A. Ullan [Espagne] ; M. J. Ward [Royaume-Uni] ; R. S. Warwick [Royaume-Uni] ; P. J. Wheatley [Royaume-Uni] ; N. A. Webb [France] ; D. Worrall [Royaume-Uni] ; W. Yuan [Royaume-Uni, République populaire de Chine] ; H. Ziaeepour [Royaume-Uni]

Source :

RBID : Pascal:08-0035961

Descripteurs français

English descriptors

Abstract

Aims. X-ray sources at intermediate fluxes (a few ×10-14 erg cm-2 s-1) with a sky density of ∼100 deg-2 2 are responsible for a significant fraction of the cosmic X-ray background at various energies below 10 keV. The aim of this paper is to provide an unbiased and quantitative description of the X-ray source population at these fluxes and in various X-ray energy bands. Methods. We present the XMM-Newton Medium sensitivity Survey (XMS), including a total of 318 X-ray sources found among the serendipitous content of 25 XMM-Newton target fields. The XMS comprises four largely overlapping source samples selected at soft (0.5-2 keV), intermediate (0.5-4.5 keV), hard (2-10 keV) and ultra-hard (4.5-7.5 keV) bands, the first three of them being flux-limited. Results. We report on the optical identification of the XMS samples, complete to 85-95%. At the flux levels sampled by the XMS we find that the X-ray sky is largely dominated by Active Galactic Nuclei. The fraction of stars in soft X-ray selected samples is below 10%, and only a few per cent for hard selected samples. We find that the fraction of optically obscured objects in the AGN population stays constant at around 15-20% for soft and intermediate band selected X-ray sources, over 2 decades of flux. The fraction of obscured objects amongst the AGN population is larger (∼35-45%) in the hard or ultra-hard selected samples, and constant across a similarly wide flux range. The distribution in X-ray-to-optical flux ratio is a strong function of the selection band, with a larger fraction of sources with high values in hard selected samples. Sources with X-ray-to-optical flux ratios in excess of 10 are dominated by obscured AGN, but with a significant contribution from unobscured AGN.


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<s1>Institute of Astronomy, Madingley Road</s1>
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<sZ>47 aut.</sZ>
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<s1>Observatoire Astronomique de Strasbourg, 11 rue de l'Université</s1>
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<s1>Max-Planck-Institut für Extraterrestrische Physik, Giessen-bachstrasse</s1>
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<inist:fA14 i1="05">
<s1>Max-Planck-Institut für Extraterrestrische Physik, Giessen-bachstrasse</s1>
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<wicri:noRegion>85740 Garching</wicri:noRegion>
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<s1>Centre for Astrophysics, University of Central Lancashire</s1>
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<s1>Astrophysikalisches Institut Potsdam, An der Sternwarte 16</s1>
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<region type="land" nuts="2">Brandebourg</region>
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<settlement type="city">Londres</settlement>
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<region type="région" nuts="1">Grand Londres</region>
</placeName>
</affiliation>
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<inist:fA14 i1="12">
<s1>South African Large Telescope, PO Box 9</s1>
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<country>Afrique du Sud</country>
<wicri:noRegion>Observatory, 7935</wicri:noRegion>
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<name sortKey="Maccacaro, T" sort="Maccacaro, T" uniqKey="Maccacaro T" first="T." last="Maccacaro">T. Maccacaro</name>
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<inist:fA14 i1="08">
<s1>INAF -Osservatorio Astronomico di Brera, via Brera 28</s1>
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<country>Italie</country>
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<s1>Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking</s1>
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<wicri:noRegion>Surrey RH5 6NT</wicri:noRegion>
<orgName type="university">University College de Londres</orgName>
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<settlement type="city">Londres</settlement>
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<region type="région" nuts="1">Grand Londres</region>
</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>
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<s1>Institute of Astronomy, Madingley Road</s1>
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<sZ>19 aut.</sZ>
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<sZ>32 aut.</sZ>
<sZ>47 aut.</sZ>
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<wicri:noRegion>Cambridge CB3 0HA</wicri:noRegion>
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<s1>Observatoire Astronomique de Strasbourg, 11 rue de l'Université</s1>
<s2>67000 Strasbourg</s2>
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<region type="region" nuts="2">Grand Est</region>
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</affiliation>
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<author>
<name sortKey="Mittaz, J P D" sort="Mittaz, J P D" uniqKey="Mittaz J" first="J. P. D." last="Mittaz">J. P. D. Mittaz</name>
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<s1>Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking</s1>
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<wicri:noRegion>Surrey RH5 6NT</wicri:noRegion>
<orgName type="university">University College de Londres</orgName>
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<settlement type="city">Londres</settlement>
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</placeName>
</affiliation>
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<author>
<name sortKey="Motch, C" sort="Motch, C" uniqKey="Motch C" first="C." last="Motch">C. Motch</name>
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<s1>Observatoire Astronomique de Strasbourg, 11 rue de l'Université</s1>
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<region type="region" nuts="2">Grand Est</region>
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<name sortKey="Negueruela, I" sort="Negueruela, I" uniqKey="Negueruela I" first="I." last="Negueruela">I. Negueruela</name>
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<s1>Observatoire Astronomique de Strasbourg, 11 rue de l'Université</s1>
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<s1>Departamento de Física, Ingeniería de Sistemas y Teoría de la Serial, Universidad de Alicante</s1>
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<country>Espagne</country>
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<name sortKey="Osborne, J P" sort="Osborne, J P" uniqKey="Osborne J" first="J. P." last="Osborne">J. P. Osborne</name>
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<inist:fA14 i1="03">
<s1>X-ray and Observational Astronomy Group, Department of Physics and Astronomy, Leicester University</s1>
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<s1>Instituto de Física de Cantabria (CSIC-UC)</s1>
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<s1>Instituto de Astrofísica de Canarias</s1>
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<country>Espagne</country>
<placeName>
<region nuts="2" type="communauté">Canaries</region>
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<s1>X-ray and Observational Astronomy Group, Department of Physics and Astronomy, Leicester University</s1>
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<inist:fA14 i1="03">
<s1>X-ray and Observational Astronomy Group, Department of Physics and Astronomy, Leicester University</s1>
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<s1>Department of Physics, University of Durham, South Road</s1>
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<sZ>41 aut.</sZ>
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<name sortKey="Rosen, S" sort="Rosen, S" uniqKey="Rosen S" first="S." last="Rosen">S. Rosen</name>
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<s1>Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking</s1>
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<s1>X-ray and Observational Astronomy Group, Department of Physics and Astronomy, Leicester University</s1>
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<name sortKey="Schartel, N" sort="Schartel, N" uniqKey="Schartel N" first="N." last="Schartel">N. Schartel</name>
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<inist:fA14 i1="16">
<s1>European Space Astronomy Centre</s1>
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<country>Espagne</country>
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<name sortKey="Schurch, N" sort="Schurch, N" uniqKey="Schurch N" first="N." last="Schurch">N. Schurch</name>
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<s1>X-ray and Observational Astronomy Group, Department of Physics and Astronomy, Leicester University</s1>
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<s1>Department of Physics, University of Durham, South Road</s1>
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<sZ>41 aut.</sZ>
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<name sortKey="Schwope, A" sort="Schwope, A" uniqKey="Schwope A" first="A." last="Schwope">A. Schwope</name>
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<inist:fA14 i1="11">
<s1>Astrophysikalisches Institut Potsdam, An der Sternwarte 16</s1>
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<region type="land" nuts="2">Brandebourg</region>
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<name sortKey="Severgnin, P" sort="Severgnin, P" uniqKey="Severgnin P" first="P." last="Severgnin">P. Severgnin</name>
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<s1>Centro de Astrobiología (CSIC-INTA), PO Box 50727</s1>
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<sZ>46 aut.</sZ>
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</inist:fA14>
<country>Espagne</country>
<placeName>
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<name sortKey="Sharp, R" sort="Sharp, R" uniqKey="Sharp R" first="R." last="Sharp">R. Sharp</name>
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<s1>Institute of Astronomy, Madingley Road</s1>
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<title xml:lang="en" level="a">The XMM-Newton serendipitous survey. IV. Optical identification of the XMM-Newton medium sensitivity survey (XMS)</title>
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<s1>Instituto de Física de Cantabria (CSIC-UC)</s1>
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<s1>Instituto de Física de Cantabria (CSIC-UC)</s1>
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<name sortKey="Pye, J P" sort="Pye, J P" uniqKey="Pye J" first="J. P." last="Pye">J. P. Pye</name>
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<name sortKey="Roberts, T P" sort="Roberts, T P" uniqKey="Roberts T" first="T. P." last="Roberts">T. P. Roberts</name>
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<s1>Anglo-Australian Observatory, PO Box 296</s1>
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<name sortKey="Stewart, G C" sort="Stewart, G C" uniqKey="Stewart G" first="G. C." last="Stewart">G. C. Stewart</name>
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<name sortKey="Szokoly, G" sort="Szokoly, G" uniqKey="Szokoly G" first="G." last="Szokoly">G. Szokoly</name>
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<s1>Max-Planck-Institut für Extraterrestrische Physik, Giessen-bachstrasse</s1>
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<author>
<name sortKey="Ullan, A" sort="Ullan, A" uniqKey="Ullan A" first="A." last="Ullan">A. Ullan</name>
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<s1>Instituto de Física de Cantabria (CSIC-UC)</s1>
<s2>39005 Santander</s2>
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<country>Espagne</country>
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<region nuts="2" type="communauté">Communauté de Madrid</region>
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<author>
<name sortKey="Ward, M J" sort="Ward, M J" uniqKey="Ward M" first="M. J." last="Ward">M. J. Ward</name>
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<s1>X-ray and Observational Astronomy Group, Department of Physics and Astronomy, Leicester University</s1>
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<country>Royaume-Uni</country>
<wicri:noRegion>Leicester LEI 7RH</wicri:noRegion>
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<affiliation wicri:level="1">
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<s1>Department of Physics, University of Durham, South Road</s1>
<s2>Durham DH1 3LE</s2>
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<country>Royaume-Uni</country>
<wicri:noRegion>Durham DH1 3LE</wicri:noRegion>
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<author>
<name sortKey="Warwick, R S" sort="Warwick, R S" uniqKey="Warwick R" first="R. S." last="Warwick">R. S. Warwick</name>
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<inist:fA14 i1="03">
<s1>X-ray and Observational Astronomy Group, Department of Physics and Astronomy, Leicester University</s1>
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<country>Royaume-Uni</country>
<wicri:noRegion>Leicester LEI 7RH</wicri:noRegion>
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<author>
<name sortKey="Wheatley, P J" sort="Wheatley, P J" uniqKey="Wheatley P" first="P. J." last="Wheatley">P. J. Wheatley</name>
<affiliation wicri:level="1">
<inist:fA14 i1="03">
<s1>X-ray and Observational Astronomy Group, Department of Physics and Astronomy, Leicester University</s1>
<s2>Leicester LEI 7RH</s2>
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<wicri:noRegion>Leicester LEI 7RH</wicri:noRegion>
</affiliation>
<affiliation wicri:level="1">
<inist:fA14 i1="19">
<s1>Department of Physics, University of Warwick</s1>
<s2>Coventry CV4 7AL</s2>
<s3>GBR</s3>
<sZ>53 aut.</sZ>
</inist:fA14>
<country>Royaume-Uni</country>
<wicri:noRegion>Coventry CV4 7AL</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Webb, N A" sort="Webb, N A" uniqKey="Webb N" first="N. A." last="Webb">N. A. Webb</name>
<affiliation wicri:level="3">
<inist:fA14 i1="20">
<s1>Centre d'Étude Spatiale des Rayonnements, CNRS/UPS, 9 avenue du Colonel Roche</s1>
<s2>31028 Toulouse</s2>
<s3>FRA</s3>
<sZ>54 aut.</sZ>
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<country>France</country>
<placeName>
<region type="region" nuts="2">Occitanie (région administrative)</region>
<region type="old region" nuts="2">Midi-Pyrénées</region>
<settlement type="city">Toulouse</settlement>
</placeName>
</affiliation>
</author>
<author>
<name sortKey="Worrall, D" sort="Worrall, D" uniqKey="Worrall D" first="D." last="Worrall">D. Worrall</name>
<affiliation wicri:level="1">
<inist:fA14 i1="04">
<s1>H.H. Wills Physics Laboratory, University of Bristol, Tyndall Avenue</s1>
<s2>Bristol BS8 1TL</s2>
<s3>GBR</s3>
<sZ>12 aut.</sZ>
<sZ>15 aut.</sZ>
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</inist:fA14>
<country>Royaume-Uni</country>
<wicri:noRegion>Bristol BS8 1TL</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Yuan, W" sort="Yuan, W" uniqKey="Yuan W" first="W." last="Yuan">W. Yuan</name>
<affiliation wicri:level="1">
<inist:fA14 i1="09">
<s1>Institute of Astronomy, Madingley Road</s1>
<s2>Cambridge CB3 0HA</s2>
<s3>GBR</s3>
<sZ>19 aut.</sZ>
<sZ>23 aut.</sZ>
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<country>Royaume-Uni</country>
<wicri:noRegion>Cambridge CB3 0HA</wicri:noRegion>
</affiliation>
<affiliation wicri:level="1">
<inist:fA14 i1="21">
<s1>National Astronomical Observatories of China/Yunnan Observatory, Phoenix Hill, PO Box 110</s1>
<s2>Kunming, Yunnan</s2>
<s3>CHN</s3>
<sZ>56 aut.</sZ>
</inist:fA14>
<country>République populaire de Chine</country>
<wicri:noRegion>Kunming, Yunnan</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Ziaeepour, H" sort="Ziaeepour, H" uniqKey="Ziaeepour H" first="H." last="Ziaeepour">H. Ziaeepour</name>
<affiliation wicri:level="4">
<inist:fA14 i1="02">
<s1>Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking</s1>
<s2>Surrey RH5 6NT</s2>
<s3>GBR</s3>
<sZ>4 aut.</sZ>
<sZ>20 aut.</sZ>
<sZ>29 aut.</sZ>
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<sZ>34 aut.</sZ>
<sZ>42 aut.</sZ>
<sZ>57 aut.</sZ>
</inist:fA14>
<country>Royaume-Uni</country>
<wicri:noRegion>Surrey RH5 6NT</wicri:noRegion>
<orgName type="university">University College de Londres</orgName>
<placeName>
<settlement type="city">Londres</settlement>
<region type="country">Angleterre</region>
<region type="région" nuts="1">Grand Londres</region>
</placeName>
</affiliation>
</author>
</analytic>
<series>
<title level="j" type="main">Astronomy and astrophysics : (Berlin. Print)</title>
<title level="j" type="abbreviated">Astron. astrophys. : (Berl., Print)</title>
<idno type="ISSN">0004-6361</idno>
<imprint>
<date when="2007">2007</date>
</imprint>
</series>
</biblStruct>
</sourceDesc>
<seriesStmt>
<title level="j" type="main">Astronomy and astrophysics : (Berlin. Print)</title>
<title level="j" type="abbreviated">Astron. astrophys. : (Berl., Print)</title>
<idno type="ISSN">0004-6361</idno>
</seriesStmt>
</fileDesc>
<profileDesc>
<textClass>
<keywords scheme="KwdEn" xml:lang="en">
<term>Active galaxies</term>
<term>Active galaxy nuclei</term>
<term>Cosmic radiation</term>
<term>Cosmic x-ray sources</term>
<term>Galaxy nuclei</term>
<term>Selection function</term>
<term>Soft X radiation</term>
<term>X-ray galaxies</term>
</keywords>
<keywords scheme="Pascal" xml:lang="fr">
<term>Rayonnement cosmique</term>
<term>Noyau galactique actif</term>
<term>Rayon X mou</term>
<term>Fonction sélection</term>
<term>Galaxies RX</term>
<term>Galaxies actives</term>
<term>Noyau galaxies</term>
<term>Source RX cosmique</term>
</keywords>
</textClass>
</profileDesc>
</teiHeader>
<front>
<div type="abstract" xml:lang="en">Aims. X-ray sources at intermediate fluxes (a few ×10
<sup>-14</sup>
erg cm
<sup>-2</sup>
s
<sup>-1</sup>
) with a sky density of ∼100 deg
<sup>-2</sup>
2 are responsible for a significant fraction of the cosmic X-ray background at various energies below 10 keV. The aim of this paper is to provide an unbiased and quantitative description of the X-ray source population at these fluxes and in various X-ray energy bands. Methods. We present the XMM-Newton Medium sensitivity Survey (XMS), including a total of 318 X-ray sources found among the serendipitous content of 25 XMM-Newton target fields. The XMS comprises four largely overlapping source samples selected at soft (0.5-2 keV), intermediate (0.5-4.5 keV), hard (2-10 keV) and ultra-hard (4.5-7.5 keV) bands, the first three of them being flux-limited. Results. We report on the optical identification of the XMS samples, complete to 85-95%. At the flux levels sampled by the XMS we find that the X-ray sky is largely dominated by Active Galactic Nuclei. The fraction of stars in soft X-ray selected samples is below 10%, and only a few per cent for hard selected samples. We find that the fraction of optically obscured objects in the AGN population stays constant at around 15-20% for soft and intermediate band selected X-ray sources, over 2 decades of flux. The fraction of obscured objects amongst the AGN population is larger (∼35-45%) in the hard or ultra-hard selected samples, and constant across a similarly wide flux range. The distribution in X-ray-to-optical flux ratio is a strong function of the selection band, with a larger fraction of sources with high values in hard selected samples. Sources with X-ray-to-optical flux ratios in excess of 10 are dominated by obscured AGN, but with a significant contribution from unobscured AGN.</div>
</front>
</TEI>
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<list>
<country>
<li>Afrique du Sud</li>
<li>Allemagne</li>
<li>Australie</li>
<li>Espagne</li>
<li>France</li>
<li>Italie</li>
<li>Royaume-Uni</li>
<li>Russie</li>
<li>République populaire de Chine</li>
</country>
<region>
<li>Alsace (région administrative)</li>
<li>Angleterre</li>
<li>Brandebourg</li>
<li>Canaries</li>
<li>Cantabrie</li>
<li>Communauté de Madrid</li>
<li>Communauté valencienne</li>
<li>Grand Est</li>
<li>Grand Londres</li>
<li>Midi-Pyrénées</li>
<li>Occitanie (région administrative)</li>
</region>
<settlement>
<li>Alicante</li>
<li>Londres</li>
<li>Potsdam</li>
<li>Strasbourg</li>
<li>Toulouse</li>
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