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| Format: | Recurso digital |
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Zenodo
2026
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| Online Access: | https://doi.org/10.5281/zenodo.19958364 |
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Table of Contents:
- <p>Inter-Model Disagreement in Kepler Exoplanet Classification: A Leakage-Aware Benchmark</p> <p>This release accompanies the submission of the paper to Astronomy and Computing (Elsevier).</p> <h2>What's included</h2> <ul> <li>IMDA.ipynb — full analysis pipeline: data preprocessing, model training, stability analysis, candidate scoring, and figure generation</li> <li>ImageRenamer.ipynb — utility notebook to copy figures with manuscript submission names (Figure_1.png etc.)</li> </ul> <h2>Reproducibility</h2> <ul> <li>Dataset: NASA Kepler KOI cumulative catalogue (cumulative.csv), January 2025 version, downloadable from https://exoplanetarchive.ipac.caltech.edu</li> <li>All results obtained with RANDOM_STATE = 42, stability seeds {0, 7, 21, 42, 99}</li> <li>Package versions documented in the first cell of IMDA.ipynb</li> </ul> <h2>Figures generated by IMDA.ipynb</h2> <ul> <li>candidate_voting.png — model voting distribution on 1979 CANDIDATE objects</li> <li>pairwise_consistency_grouped.png — pairwise model consistency by decision boundary type</li> <li>feature_correlation.png — Pearson correlation matrix for 12 transit features</li> <li>feature_importance_permutation.png — permutation importance (Random Forest)</li> <li>feature_importance_impurity.png — impurity-based importance (Random Forest)</li> <li>confusion_matrices.png, roc_curves.png, calibration_curves.png</li> <li>candidate_zones_scatter.png, grey_zone_hexbin.png</li> </ul> <h2>Manuscript figure mapping</h2> <p>Run ImageRenamer.ipynb to generate submission-ready copies:</p> <ul> <li>feature_correlation.png → Figure_1.png</li> <li>feature_importance_permutation.png → Figure_2a.png</li> <li>feature_importance_impurity.png → Figure_2b.png</li> <li>candidate_voting.png → Figure_3.png</li> <li>pairwise_consistency_grouped.png → Figure_4.png</li> </ul>