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Reconstructing the Projected Dark Matter Field across 0.1–100 Mpc Scales from the SDSS Survey

  • Authors: Kunyao Zhao, Yingjie Peng, Dingyi Zhao, Xiaohu Yang, Luis C. Ho, Kai Wang, Jing Dou, Zeyu Gao, Qiusheng Gu, Yukun Liu, Roberto Maiolino, Houjun Mo, Alvio Renzini, Canpo Su, Bitao Wang, Yu-Chen Wang, Bingxiao Xu, Feng Yuan, Xingye Zhu

Kunyao Zhao et al 2026 The Astrophysical Journal Letters 1010 .

  • Provider: AAS Journals

Caption: Figure B1.

Validation of the projected-aperture-based halo mass estimates after including fiber collisions and stellar-mass uncertainties in IllustrisTNG300-1. Left: comparison between the projected-aperture masses integrated within R200 in the ground-truth and reconstructed projected matter maps. Blue points denote individual dark matter halos, and black contours show their number density distribution. The red line shows the mean reconstructed projected-aperture mass in bins of the true projected-aperture mass, with error bars indicating the standard deviation. The black dashed line denotes the one-to-one relation. In the inset, the red and green lines show the mean (μ) and standard deviation (σ) of the residuals in each true projected-aperture-mass bin, respectively, while the gray dashed lines mark ±0.3 dex. Right: comparison between the reconstructed projected-aperture mass within R200 and the catalog mass M200. Visual conventions follow those used in the left panel.

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