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Nowhere Left to Hide: Revealing Realistic Gravitational-wave Populations in High Dimensions and High Resolution with PixelPop

  • Authors: Sofía Álvarez-López, Jack Heinzel, Matthew Mould, Salvatore Vitale

Sofía Álvarez-López et al 2026 The Astrophysical Journal Letters 1006 .

  • Provider: AAS Journals

Caption: Figure 11.

Inferred merger-rate density ﹩{ \mathcal R }({\chi }_{{\rm{eff}}};z)﹩ at redshifts z = 0.2 (left, in blue) and z = 0.8 (right, in orange) with the PEAK + TUKEY model on the population with artificially removed correlations. Compared to Figure 4, the true distribution (dashed lines) is now within the 99% credible interval (shaded gray region) of the inferred rate.

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