The XMM-Large scale structure catalogue:: X-ray sources and associated optical data.: Version I

被引:57
作者
Pierre, M. [1 ]
Chiappetti, L.
Pacaud, F.
Gueguen, A.
Libbrecht, C.
Altieri, B.
Aussel, H.
Gandhi, P.
Garcet, O.
Gosset, E.
Paioro, L.
Ponman, T. J.
Read, A. M.
Refregier, A.
Starck, J. -L.
Surdej, J.
Valtchanov, I.
Adami, C.
Alloin, D.
Alshino, A.
Andreon, S.
Birkinshaw, M.
Bremer, M.
Detal, A.
Duc, P. -A.
Galaz, G.
Jones, L.
Le Fevre, J. -P.
Le Fevre, O.
Maccagni, D.
Mazure, A.
Quintana, H.
Rottgering, H. J. A.
Sprimont, P. -G.
Tasse, C.
Trinchieri, G.
Willis, J. P.
机构
[1] Univ Paris 06, CEA Saclay, Serv Astrophys, DAPNIA,DSM,Lab AIM,CNRS, F-91191 Gif Sur Yvette, France
[2] IASF Milano, INAF, I-20133 Milan, Italy
[3] ESA, Villafranca Del Castillo, Spain
[4] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England
[5] Univ Liege, Inst Astrophys & Geophys, B-4000 Sart Tilman Par Liege, Belgium
[6] Univ Birmingham, Sch Phys & Astron, Birmingham B15 2TT, W Midlands, England
[7] Univ Leicester, Dept Phys & Astron, Leicester LE1 7RH, Leics, England
[8] SEDI CEA Saclay, DAPNIA, F-91191 Gif Sur Yvette, France
[9] Lab Astrophys Marseille, Marseille, France
[10] Osserv Astron Brera, INAF, Milan, Italy
[11] Univ Bristol, Dept Phys, Bristol BS8 1TL, Avon, England
[12] Pontificia Univ Catolica Chile, Dept Astron & Astrofis, Santiago, Chile
[13] Leiden Observ, NL-2300 RA Leiden, Netherlands
[14] Univ Victoria, Dept Phys & Astron, Victoria, BC V8P 1A1, Canada
基金
英国科学技术设施理事会;
关键词
catalogues; surveys; X-rays; general;
D O I
10.1111/j.1365-2966.2007.12354.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Following the presentation of the XMM-Large Scale Structure (XMM-LSS) survey X-ray source detection package by Pacaud et al., we provide the source lists for the first surveyed 5.5 deg(2). The catalogues pertain to the [0.5-2] and [2-10] keV bands and contain in total 3385 pointlike or extended sources above a detection likelihood of 15 in either band. The agreement with deep log N-log S is excellent. The main parameters considered are position, count rate, source extent with associated likelihood values. A set of additional quantities such as astrometric corrections and fluxes are further calculated while errors on the position and count rate are deduced from simulations. We describe the construction of the band-merged catalogue allowing rapid subsample selection and easy cross-correlation with external multiwavelength catalogues. A small optical Canada-France-Hawaii Telescope Legacy Survey multiband subset of objects are associated with each source along with an X-ray/optical overlay. We make the full X-ray images available in FITS format. The data are available at the Centre de Donnees de Strasbourg and, in a more extended form, at the Milan XMM-LSS survey data base.
引用
收藏
页码:279 / 290
页数:12
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