The XMM-LSS survey -: The XMDS/VVDS 4σ catalogue

被引：51

作者：

Chiappetti, L

Tajer, M

Trinchieri, G

Maccagni, D

Maraschi, L

Paioro, L

Pierre, M

Surdej, J

Garcet, O

Gosset, E

Le Fèvre, O

Bertin, E

McCracken, HJ

Mellier, Y

Foucaud, S

Radovich, M

Ripepi, V

Arnaboldi, M

机构：

[1] IASF, INAF, Sez Milano G Occhialini, I-20133 Milan, Italy

[2] Observ Brera, INAF, I-20121 Milan, Italy

[3] CEA, DSM, DAPNIA, Serv Astrophys, F-91191 Gif Sur Yvette, France

[4] Univ Liege, Inst Astrophys & Geophys, B-4000 Liege, Belgium

[5] Univ Milan, Dipartimento Fis, I-20126 Milan, Italy

[6] Lab Astrophys Marseille, F-13376 Marseille, France

[7] Inst Astrophys, F-75014 Paris, France

[8] Osserv Astron Capodimonte, INAF, I-80131 Naples, Italy

[9] Osserv Astron Torino, INAF, I-10025 Pino Torinese, Italy

来源：

ASTRONOMY & ASTROPHYSICS | 2005年 / 439卷 / 01期

关键词：

X-ray : general; surveys; quasars : general; catalogs;

D O I：

10.1051/0004-6361:20042583

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present a first catalogue of X-ray sources resulting from the central area of the XMM-LSS (Large Scale Structure survey). We describe the reduction procedures and the database tools we developed and used to derive a well defined catalogue of X-ray sources. The present catalogue is limited to a sub-sample of 286 sources detected at 4 sigma in the 1 deg(2) area covered by the photometric VVDS (VIRMOS VLT Deep Survey), which allows us to provide optical and radio identifications. We also discuss the X-ray properties of a larger X-ray sample of 536 sources detected at > 4 sigma in the full 3 deg(2) area of the XMM Medium Deep Survey (XMDS) independently of the optical identification. We also derive the log N - log S relationship for a sample of more than one thousand sources that we discuss in the context of other surveys at similar fluxes.

引用

页码：413 / U126

页数：16

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