弱透镜质量图中的峰值用于星团天体物理学和宇宙学
Masamune Oguri1,2, Satoshi Miyazaki3,4
1Center for Frontier Science, Chiba University, Inage-ku, Chiba, Japan.
概括
弱引力透镜通过质量来识别星系团,为宇宙学研究提供了强大的方法. 这种方法与传统方法不同,提高了集群丰度测量的准确性.
科学领域:
- 宇宙学的宇宙学是什么?
- 天体物理学 天体物理学
背景情况:
- 传统上,星系团的选择是基于其微子属性.
- 弱引力透镜提供了一个替代的,纯粹的引力选择方法.
研究的目的:
- 审查弱透镜剪切选择集群样本的基础和应用.
- 突出重力选择如何有助于强大的宇宙学约束导出.
主要方法:
- 从剪切目录中构建弱透镜光圈质量图.
- 在这些质量图中,将星系团识别为峰值.
- 对剪切选择集群的微子特性进行分析.
主要成果:
- 在Subaru Hyper Suprime-Cam调查中发现了300多个剪切选择集群 (S/N > 5).
- 纯引力选择允许更容易,更强大的选择函数的量化.
- 对バリオン属性的研究为星团天体物理学提供了新的见解.
结论:
- 弱透镜剪切选择集群对于准确的宇宙学约束至关重要.
- 在宇宙学分析中,系统效应可以通过仔细选择分析参数来减轻.
- 这种方法为我们进一步了解星系团和宇宙提供了一个强大的工具.
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