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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 6.

Inferred merger-rate density ﹩{ \mathcal R }({\chi }_{{\rm{eff}}};z)﹩ evaluated at redshifts z = 0.2 (blue) and z = 0.8 (orange) for three-dimensional PIXELPOP (left) and the HYBRID model (right), defined in Equations (6) and (7), respectively. The dashed line shows the true population, while the solid line and shaded region represent the posterior median and central 90% credible region.

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