The CFHTLS strong lensing legacy survey I.: Survey overview and T0002 release sample

被引:152
作者
Cabanac, R. A.
Alard, C.
Dantel-Fort, M.
Fort, B.
Gavazzi, R.
Gomez, P.
Kneib, J. P.
Le Fevre, O.
Mellier, Y.
Pello, R.
Soucail, G.
Sygnet, J. F.
Valls-Gabaud, D.
机构
[1] Canada France Hawaii Telescope Corp, Kamuela, HI 96743 USA
[2] Observ Paris, CNRS, UMR 8112, LERMA, F-75014 Paris, France
[3] Inst Astrophys, CNRS, UMR 7095, F-75014 Paris, France
[4] Univ Paris 06, F-75014 Paris, France
[5] Lab Astrophys Toulouse Tarbes, CNRS, UMR5572, F-31400 Toulouse, France
[6] Univ Toulouse 3, F-31400 Toulouse, France
[7] Gemini Observ, No Operat Ctr, Hilo, HI 96720 USA
[8] Lab Astrophys Marseille, F-13376 Marseille 12, France
[9] Observ Paris, CNRS, GEPI, UMR 8111, F-92195 Meudon, France
来源
ASTRONOMY & ASTROPHYSICS | 2007年 / 461卷 / 03期
关键词
gravitational lensing; surveys; cosmology : dark matter; galaxies : fundamental parameters; galaxies : clusters : general; galaxies : halos;
D O I
10.1051/0004-6361:20065810
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Aims. We present data from the CFHTLS Strong Lensing Legacy Survey (SL2S). Due to the unsurpassed combined depth, area and image quality of the Canada-France-Hawaii Legacy Survey it is becoming possible to uncover a large, statistically well-defined sample of strong gravitational lenses which spans the dark halo mass spectrum predicted by the concordance model from galaxy to cluster haloes. Methods. We describe the development of several automated procedures to find strong lenses of various mass regimes in CFHTLS images. Results. The preliminary sample of about 40 strong lensing candidates discovered in the CFHTLS T0002 release, covering an effective field of view of 28 deg(2) is presented. These strong lensing systems were discovered using an automated search and consist mainly of gravitational arc systems with splitting angles between 2 and 15 arcsec. This sample shows for the first time that it is possible to uncover a large population of strong lenses from galaxy groups with typical halo masses of about 10(13) h(-1) M-circle dot. We discuss the future evolution of the SL2S project and its main scientific aims for the next 3 years, in particular our observational strategy to extract the hundreds of gravitational rings also present in these fields.
引用
收藏
页码:813 / 821
页数:9
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