首页> 外文会议>International Astronomical Union >Higher Order Cross-Correlation Functions from Galaxy-Galaxy-Galaxy Lensing
【24h】

Higher Order Cross-Correlation Functions from Galaxy-Galaxy-Galaxy Lensing

机译:Galaxy-Galaxy-Galaxy透镜的高阶交叉相关功能

获取原文

摘要

Galaxy-galaxy lensing (GGL) measures the 2-point cross-correlation between galaxies and mass in the universe. In this work we seek to generalise this effect by considering the third-order correlations between galaxies and mass: galaxy-galaxy-galaxy lensing We introduce the higher-order cross-correlation functions and discuss their physical interpretation in terms of the halo model We then demonstrate that measuring the lensing shear of background galaxies about foreground galaxy pairs, which we term galaxy-galaxy-galaxy lensing, provides a measure of the third-order cross functions We note that current surveys in which detections of the cosmic shear 3-point correlation function have been reported should also be able to detect galaxy-galaxy-galaxy lensing Indeed, we suggest that this effect may already have been detected in recent studies of GGL
机译:Galaxy-Galaxy镜头(GGL)测量宇宙中的星系与群众之间的2点交叉相关性。在这项工作中,我们寻求通过考虑星系与质量之间的三阶相关性:Galaxy-Galaxy-Galaxy镜头的三阶相关性,我们介绍了更高阶的互相关功能,并在我们的Halo模型方面讨论它们的物理解释证明测量关于前台星系对的背景星系的镜片剪切,我们术语Galaxy-Galaxy-Galaxy镜头提供了三阶交叉功能的量度,我们注意到电流调查,其中宇宙剪切3点相关的检测据报道,功能还应该能够检测到Galaxy-Galaxy-Galaxy镜片的实际上,我们表明在最近对GGL的研究中可能已经检测到这种效果

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号