Observer-Normalized Scale Coherence II: Execution of a Pre-Registered Prediction in the Dwarf Galaxy Regime
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2026
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| _version_ | 1866901786520977408 |
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| author | Brown, Jason |
| author_facet | Brown, Jason |
| contents | <p>This repository contains the data, code, and outputs supporting <em>Observer-Normalized Scale Coherence II: Execution of a Pre-Registered Prediction in the Dwarf Galaxy Regime</em>.</p> <p>The analysis executes a pre-registered, zero-parameter prediction defined in Paper I, applying frozen definitions to a dwarf-galaxy subset drawn from the SPARC database. No fitting, tuning, or renormalization is performed.</p> <p>The predicted relation holds in the dwarf regime with a log-scatter of approximately 0.16–0.18 dex, consistent with the observational scatter limit and statistically indistinguishable from that observed in the spiral-galaxy calibration sample. Residuals show no systematic dependence on mass, radius, or velocity.</p> <p>Included are the manuscript PDF, the Python analysis script, the SPARC input data used, and all generated tables and figures required for full reproduction of the results.</p> |
| format | Recurso digital |
| id | zenodo_https___doi_org_10_5281_zenodo_18308167 |
| institution | Zenodo |
| language | |
| publishDate | 2026 |
| publisher | Zenodo |
| record_format | zenodo |
| spellingShingle | Observer-Normalized Scale Coherence II: Execution of a Pre-Registered Prediction in the Dwarf Galaxy Regime Brown, Jason SPARC Galaxy Dynamics Dwarf Galaxies Dark Matter Discrepancy Scale Coherence Pre-Registered Prediction <p>This repository contains the data, code, and outputs supporting <em>Observer-Normalized Scale Coherence II: Execution of a Pre-Registered Prediction in the Dwarf Galaxy Regime</em>.</p> <p>The analysis executes a pre-registered, zero-parameter prediction defined in Paper I, applying frozen definitions to a dwarf-galaxy subset drawn from the SPARC database. No fitting, tuning, or renormalization is performed.</p> <p>The predicted relation holds in the dwarf regime with a log-scatter of approximately 0.16–0.18 dex, consistent with the observational scatter limit and statistically indistinguishable from that observed in the spiral-galaxy calibration sample. Residuals show no systematic dependence on mass, radius, or velocity.</p> <p>Included are the manuscript PDF, the Python analysis script, the SPARC input data used, and all generated tables and figures required for full reproduction of the results.</p> |
| title | Observer-Normalized Scale Coherence II: Execution of a Pre-Registered Prediction in the Dwarf Galaxy Regime |
| topic | SPARC Galaxy Dynamics Dwarf Galaxies Dark Matter Discrepancy Scale Coherence Pre-Registered Prediction |
| url | https://doi.org/10.5281/zenodo.18308167 |