Kaileh57/opacity-marginalization
Amortized opacity marginalization: data Training sets, trained models, priors and held-out evaluation sets for Amortized Opacity Marginalization Improves C/O Interval Calibration for Brown-Dwarf Retrievals (Heraty 2026, arXiv:2609.01665). Code and paper source: github.com/kaileh57/opacity-marginalization. Contents spectra/v7_opmarg: one million simulated NIRSpec G395H spectra generated with randomized molecular opacities (the marginalized training set)… See the full description on the dataset page: https://huggingface.co/datasets/Kaileh57/opacity-marginalization.
Amortized opacity marginalization: data
Training sets, trained models, priors and held-out evaluation sets for Amortized Opacity Marginalization Improves C/O Interval Calibration for Brown-Dwarf Retrievals (Heraty 2026, arXiv:2609.01665). Code and paper source: github.com/kaileh57/opacity-marginalization.
Contents
spectra/v7_opmarg: one million simulated NIRSpec G395H spectra generated with randomized molecular opacities (the marginalized training set)spectra/v6_cloud: one million matched spectra at fixed nominal opacities (the control training set)spectra/ablation_train: the one-axis training sets (discrete_only,smooth_only) behind the training-side ablationspectra/v7_opmarg_validation,spectra/v6_cloud_val: validation splitsspectra/ablation_test,spectra/broadening_test,spectra/opmarg_ampsweep_v2: the one-axis, broadening-stress and amplitude-robustness evaluation setsheldout/clean,heldout/perturbed: the held-out sets behind every reported coverage numbermodels/: trained normalizing-flow posterior estimators, comprising three marginalized seeds, three control seeds, three mask-augmented seeds, and the ablation and leave-one-out variantsreal_inputs/: preprocessed JWST NIRSpec G395H arrays (observed flux, error, bad-pixel mask per object) used for the real-data resultsresults_gcs/: evaluation outputs from the final, amplitude-robustness, broadening and recalibration-benchmark runspriors/interlist_ratio_priors_v1.json: the opacity-perturbation prior
Spectra are HDF5 shards of 128 spectra each, with parameters, flux and noise-free flux per shard. Models are PyTorch checkpoints; loading them requires zuko (see the code repository).
License
CC BY 4.0.
Citation
See the code repository for the BibTeX entry.
