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WISE/CatWISE Constraints on Dysonian Waste-heat Technosignatures in Nearby Galaxies

  • Authors: Bo-Lun Huang, Zhen-Zhao Tao, Tong-Jie Zhang

Bo-Lun Huang et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 11.

Median bias vs. injected L wh at T = 300 K, split by host SED family. Positive bias at low L wh is the expected behavior of a cap estimator in the presence of nondetections (floor at ≈) and unsubtracted host MIR continuum. The three SED families converge toward small bias at high L wh. As expected, the bias is largest for SB at the faint end (strongest MIR continuum) and decreases toward small values at high L wh, where the cap floor is negligible relative to the injected signal.

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