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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 13.

Inferred marginalized merger-rate density ﹩{ \mathcal R }({\chi }_{{\rm{eff}}};z)﹩ at redshifts z = 0.2 (blue) and z = 0.8 (orange) for the three-dimensional PIXELPOP (left) and HYBRID (right) models, using the catalog of point-estimate events. Otherwise, similar to Figure 6. In this case, any deviation from the truth in the peak of the effective spin distribution at χeff ≈ 0 is minimal. However, there is significant bias at z = 0.8 in the 0 < χeff ≤ 0.5 region.

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