Integral-Field Spectroscopy of SLACS Lenses

O. Czoske, M. Barnabè, L. Koopmans
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Abstract

The combination of two‐dimensional kinematics and gravitational lens modelling permits detailed reconstruction of the phase‐space structure of early‐type galaxies and sets constraints on the dark‐matter distribution in their inner regions. We describe a project which combines integral‐field spectroscopy from an ESO Large Programme using VIMOS on the VLT with deep HST ACS and NICMOS images to study a sample of 17 early‐type lens galaxies at z≈0.1–0.3, drawn from the Sloan Lens ACS survey (SLACS).
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slac透镜的积分场光谱
二维运动学和引力透镜模型的结合允许详细重建早期星系的相空间结构,并对其内部区域的暗物质分布设置限制。我们描述了一个项目,该项目结合了ESO大型项目的积分场光谱,使用VLT上的VIMOS与深HST ACS和NICMOS图像,研究了从斯隆透镜ACS巡天(SLACS)中提取的z≈0.1-0.3的17个早期透镜星系样本。
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