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A Calibrated Bayesian Search for Potential Chemical Technosignatures in Polluted White Dwarfs

  • Authors: Bo-Lun Huang, 博伦 黄, Zhen-Zhao Tao, 振钊 陶, Tong-Jie Zhang, 同杰 张

Bo-Lun Huang et al 2026 The Astrophysical Journal 1006 .

  • Provider: AAS Journals

Caption: Figure 5.

Injection–recovery detection power is dominated by element richness. Strong-evidence detection power, i.e., ﹩P(\mathrm{ln}{\rm{BF}}\gt \mathrm{ln}10| {\alpha }_{{\rm{true}}})﹩, is plotted against the injected Ca-normalized mixing fraction αtrue. Curves show recovery for all records together and after stratifying by the number of detected elements ﹩{N}_{{\rm{\det }}}﹩. (a), Photospheric track (atm). (b), Diffusion-adjusted track (acc_ss).

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