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Population Stability Index Calculator

The population stability index between a reference distribution and a current one — the standard drift score for model inputs and scores — with the per-bin contributions that show where the shift is.

Bin the variable the same way in both samples and compare the share in each bin.

Results update as you type
Results
Population stability index
0.03271
Reading
Bins
Bin contributing most
Its share of the PSI
Largest change in share (points)
Contribution per bin
Shares sum to (reference / current)
Reviewed September 2026. Model arithmetic is the same everywhere: the same formulas in every market, in your own currency. The NIST framework is voluntary guidance; it does not prescribe cost or sizing methods.
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About population stability index

How the population stability index calculator works

Bin the variable the same way in both samples and compare the share in each bin. PSI sums, over bins, the change in share times the log of the ratio: bins that grew or shrank a lot contribute most. Under 0.1 is stable; 0.1 to 0.25 is worth watching; above 0.25 the population has shifted and the model needs a look.

It is symmetric, dimensionless and cheap, which is why it has been the monitoring default since credit scoring — and why a spike in it is usually the first sign a model is drifting.

Formula: PSI = Σ (actualᵢ − expectedᵢ) × ln(actualᵢ / expectedᵢ)

Worked examples

InputsPopulation stability indexNote
A mild shift to the right0.03271PSI about 0.03 — stable
No change0exactly zero
A collapsed tail0.44898well over 0.25

Frequently asked questions

What is the population stability index?

A score for how much a distribution has shifted between two samples, computed from binned shares. It came from credit scoring and is now the default drift metric for model monitoring.

What thresholds should I use?

The conventional ones: under 0.1 stable, 0.1 to 0.25 moderate, above 0.25 significant. They are rules of thumb; a stricter model deserves stricter lines.

How many bins?

Ten is the norm, often deciles of the reference sample. Too few bins hide shifts; too many make small samples noisy.

Why the epsilon?

An empty bin would give a log of zero. A tiny floor keeps the math finite and barely changes the answer; a bin that goes from 10% to 0% still scores very high.

Is PSI the same as KL divergence?

It is the symmetric sum of the two KL divergences. Same idea, made symmetric so it does not matter which sample is the reference.

Where these figures come from

Last checked: September 2026. The relationships here are architectural, not vendor-specific: bytes per parameter follow the numeric format, KV-cache size follows the transformer definition, and token-per-word ratios come from published tokeniser behaviour.