Validate whether recovered posterior modes are genuine degenerate solutions

Establish whether all composition and grain-size modes recovered by TNFlow correspond to genuine degenerate solutions by resynthesizing each mode through the Shkuratov radiative transfer model and comparing the resulting spectra with the input spectrum.

Background

TNFlow produces multimodal posterior distributions over TNO surface compositions and grain sizes, and the authors identify multiple distinct solutions for most synthetic test and out-of-distribution spectra. Although the posterior often contains a mode close to the true composition, the reported mode search alone does not demonstrate that every recovered mode is physically valid or spectrally equivalent to the input.

The proposed unresolved validation is to pass each recovered mode through the forward Shkuratov radiative transfer model and compare the synthesized spectrum against the original spectrum. This would determine whether the modes represent genuine inverse-problem degeneracies rather than spurious posterior solutions.

References

The relatively accurate top-mode TV distance indicates these may also be close solutions, but establishing that all found modes are genuine degenerate solutions requires resynthesizing each mode through the forward model, which we leave to future work.

TNFlow: Amortized Posterior Inference for Trans-Neptunian Object Surface Composition  (2609.04305 - Gaur et al., 3 Sep 2026) in Section 5, Discussion