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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 15.

Inferred evolution of the merger-rate density ﹩{ \mathcal R }({\chi }_{{\rm{eff}}};z)﹩ over redshift and as a function of the effective spin χeff ≈ 0 (top), 0.05 (middle), and 0.2 (bottom). The inferred median and central 90% credible region are given by the solid line and shaded areas, respectively, while the underlying evolution of the true population is given by the dashed black line.

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