Public prototype / Phase Tuner interface

Phase Detector

Input SPARC-style galaxy data, compare it to the closest RBFL reference profile, and generate a provisional phase-alignment readout with outer-rim diagnostics, prediction prompts, and a central-object estimate.

Boundary: this is a public demonstration interface. It is designed for exploration, teaching, and pre-screening. It is not a substitute for source SPARC reductions, peer review, or the research-grade Phase Tuner.

AI radio-style phase detector machine with glowing lens and console
Detector onlineSPARC-style input ready
01Input data

Paste radius, observed velocity, baryonic velocity, and uncertainty if available.

02Reference match

The detector searches the bundled galaxy library for the closest reference profile.

03Phase readout

It estimates alignment, coherence, drift, outer-rim separation, and spike behaviour.

04Predictions

It returns phase implications, outer-rim tests, binary-star bridge prompts, and caveats.

SPARC-style input

Run a provisional phase alignment

Paste clean rotation-curve rows below. The detector runs entirely inside your browser; the public site does not upload or store your data.

Input console

Required fields

Minimum required columns: radius_kpc, vobs_kms, vbar_kms. Optional: err_kms, vgas, vdisk, vbulge. Comma, tab, or whitespace-separated rows are accepted.
Ready for SPARC-style input.
Results overview

Awaiting data

Reference: -
Phase alignment--Waiting
Phase grouping--Not calculated
Outer-rim gap----
Central object----
Paste data or load the sample to generate detector output.
Phase implication

No phase implication yet.

Outer-rim prediction

No outer-rim prediction yet.

Binary-star bridge

No binary-star bridge yet.

Central-object caution

The detector cannot identify a single central star from rotation data alone. It estimates a central-object class from inner-radius velocity behaviour.

Recommended validation checks
  • Load or paste a galaxy to see validation prompts.
Data qualityAwaiting input

Use at least 8 radial points where possible, with uncertainty columns and a clear baryonic proxy.

CSV

Data format guide

Paste one row per radial sample. Header names are flexible, but the detector needs radius, observed rotation velocity, and a baryonic velocity proxy.

radius_kpc,vobs_kms,vbar_kms,err_kms
0.50,42,38,5
1.00,75,68,5
2.00,118,100,6
RBFL

What the detector calculates

It compares your input to the closest bundled reference shape, estimates baryonic alignment, outer-rim separation, coherence, residual stress, and spike-like behaviour, then assigns a provisional phase grouping.

The output is a navigation layer. It should guide deeper analysis, not replace full reproducibility work.

From public interface to research engine

Phase Detector is the front door to the Phase Tuner idea.

The long-term goal is to connect this interface to verified SPARC tables, uncertainty envelopes, RBFL reproducibility outputs, and downloadable per-galaxy reports.

Open Galaxy Phase Map