Observable detail · GAL

UDG dynamics (NGC 1052-DF2/DF4)

Prediction / mechanismNGC 1052-DF2/DF4 ultra-diffuse galaxies show low \(\sigma_v\); DCT predicts the observed kinematics from the Avrami profile.
Measuredvan Dokkum 2018 NGC 1052-DF2 dynamics.
Residual / statusSOFT
StatusSOFT
Source paperDCT-DM-01

Mechanism

Avrami P(g) profile reproduces the low velocity dispersion at high mass-to-light ratio.

Derivation

The derivation chain follows the cluster paper DCT-DM-01 and reduces to the canonical DCT constants (\(P_0 = 0.851\), \(\omega_0 = 50{,}037\), \(c_{BD} = 138{,}189\), master identity \(2\omega_0 + 3 = c_{BD} \cdot P_0^2 = 100{,}077\)). See the cluster paper for the full multi-line derivation.

Methodology

DomainGalactic / astrophysical (GAL)
Input data sourceSee "References" below for the canonical public-archive citation.
Measurement procedureThe measured value used here is the most recent peer-reviewed central value plus 1σ uncertainty from the cited reference.
Acceptance thresholdHIT: residual within 1σ of measurement. SOFT: directional agreement within bracketing range. OPEN: untested or unresolved.
Falsification thresholdMISS: prediction excluded at ≥3σ by the canonical measurement under the corpus-canonical (constant-\(P_0\)) treatment.
Current statusSee verdict pill above.

Python verification

Verification script: astrophysical_tests.py. Run with python3 astrophysical_tests.py to reproduce the canonical DCT result against the public-archive measurement source listed below.

Cross-references

Related observables: sparc-rar · dwarf-core-cusp.

Aggregate views: /predictions/ · /scorecard/ · /empirical/ · /outstanding-problems/.

Audit notes

This sub-page is part of the post-build-out of the observable archive (see the observable index). Verdict reflects the corpus-canonical (constant-\(P_0\)) treatment. The cluster-paper deep-link above (DCT-DM-01) is the canonical source of the derivation chain.

References

Back to all observables or the predictions table.