检测到一个群体的亚毫米亮度,强烈的透镜星系
Mattia Negrello1, R Hopwood, G De Zotti
1Department of Physics and Astronomy, The Open University, Walton Hall, Milton Keynes, MK7 6AA, UK. m.negrello@open.ac.uk
概括
在亚毫米测量中检测引力透镜现在简单而有效. 早期的赫歇尔天体物理特拉赫兹大面积调查数据显示,识别这些宇宙现象的成功率很高.
科学领域:
- 天体物理学 天体物理学
- 宇宙学的宇宙学是什么?
背景情况:
- 引力透镜是研究星系和宇宙的关键工具.
- 在大型数据集中识别镜头传统上是耗时的.
- 亚毫米波长对于观测尘土的恒星形成星系至关重要.
研究的目的:
- 为了证明大面积亚毫米测量在检测引力透镜中的效率.
- 为了简化这些天文物体的识别过程.
主要方法:
- 利用了来自赫歇尔天体物理特拉赫兹大面积调查的早期数据.
- 分析了微毫米测量数据,以寻找引力透镜的信号.
主要成果:
- 成功检测出强大的重力透镜事件,效率高.
- 展示了使用大面积亚毫米调查检测的简单性和方便性.
结论:
- 广泛的亚毫米测量对于识别引力透镜是有效的.
- 这种方法大大减少了用于透镜检测所需的时间和精力.
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