Accounting for radial correlations in SPARC rotation curves as nuisance parameters eliminates the preference for pISO over NFW dark matter halo models.
MNRAS000, 1–15 (2025) Correlated rotation curves & mass models13 Figure A2.As Fig
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.GA 1years
2025 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
Consequences of radially correlated rotation curves for galaxy mass models
Accounting for radial correlations in SPARC rotation curves as nuisance parameters eliminates the preference for pISO over NFW dark matter halo models.