Image Details

Choose export citation format:

Observational Evidence for the Kinematic Memory of Cosmic Filaments from Satellite Orbital Orientations

  • Authors: Peng Wang, 鹏 王, Wei Wang, 伟 王, Wenting Wang, 文婷 王, Min Bao, 敏 鲍, Xi Kang, 熙 康, Hong Guo, 宏 郭, Youcai Zhang, 友财 张, Xiao-xiao Tang, 潇潇 唐

Peng Wang et al 2026 The Astrophysical Journal Letters 1008 .

  • Provider: AAS Journals

Caption: Figure 3.

Disentangling the primary drivers of the signal. Similar to Figure 2, but in each panel the sample is subdivided by projected distance to the nearest filament into three bins: Dfil < 0.5 h−1 Mpc (blue), 0.5 ≤ Dfil < 1.0 h−1 Mpc (orange), and 1.0 ≤ Dfil < 10.0 h−1 Mpc (green); the legend reports the number of systems in each bin. The gray dashed line marks the isotropic expectation (〈θ〉 = 45). Points show the binned mean values of the angle θ between the satellite orbital-normal vector ﹩{\hat{{\boldsymbol{n}}}}_{{\rm{orb}}}﹩ and the projected filament direction ﹩{\hat{{\boldsymbol{e}}}}_{{\rm{fil}}}﹩, and error bars indicate the 1σ uncertainty on the mean estimated from bootstrap resampling.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse