Properties of high-Z galaxies seen through lensing clusters

被引：4

作者：

Pelló, R

Bolzonella, M

Campusano, LE

Dantel-Fort, M

Fort, B

Kneib, JP

Le Borgne, JF

Mellier, Y

Ellis, RS

Smail, I

机构：

[1] Observ Midi Pyrenees, UMR 5572, F-31400 Toulouse, France

[2] Ist Fis Cosm G Occhialini, I-20133 Milan, Italy

[3] Univ Chile, Dept Astron, Observ Cerro Calan, Santiago, Chile

[4] Observ Paris, DEMIRM, F-75014 Paris, France

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

[6] CALTECH, Pasadena, CA 91125 USA

[7] Univ Durham, Dept Phys, Durham DH1 3LE, England

来源：

ASTROPHYSICS AND SPACE SCIENCE | 2001年 / 277卷 / Suppl 1期

关键词：

High-z galaxies; Gravitational Lensing;

D O I：

10.1023/A:1012795704908

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present new results obtained on the identification and study of high-z galaxies seen through lensing clusters used as gravitational telescopes. The amplification effect provides a tool to study the spectrophotometric and morphological properties of such galaxies 1 to 3 magnitudes deeper with respect to field surveys. Distant sources with 1 less than or equal to z less than or equal to 7 typically are selected close to the critical lines in clusters where the mass distribution is well known, using photometric redshifts computed on a large wavelength interval, as well as lens-inversion criteria. We focus here on the recent results obtained on AC114 and MS1008-1224, two lensing clusters at z = 0.31.

引用

页码：547 / 550

页数：4

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