Imagine two teams reconstruct the same underground structure from the same seismic data, and both report the identical best-fit image. Are the two answers equally trustworthy? Not necessarily — and the image alone cannot tell you. One team's answer might be pinned down tightly by the data; the other's might be a near-guess propped up by regularization. The difference — the error bars — is the whole point of a Bayesian treatment.
The
This single matrix is the uncertainty of the answer. Its diagonal entries are the variances of each recovered parameter — square-root them for error bars. Its off-diagonals say which parameters are correlated, i.e. which trade off against each other in the fit.
A covariance matrix is a table you can read at a glance once you know the code. For a two-parameter
model
Read off what each of these posterior covariances is telling you.
Large posterior variance is the signature of the
The posterior is a
Two ways to shrink it: gather more data (each measurement adds to the precision
The ellipse is the posterior covariance for a two-parameter model. With few measurements it is large and tilted (high, correlated uncertainty). Add measurements with the slider: each one adds precision, and the ellipse contracts — fastest along the well-measured direction, slowest along the poorly-measured one, so it does not just shrink but changes shape.
A reconstruction's mean alone is dangerously incomplete without its posterior covariance. Two reconstructions can look pixel-for-pixel identical yet have wildly different reliability — one tightly constrained by data, the other a soft guess held up by regularization. Reporting an estimate with no covariance is like reporting a measurement with no error bars: it looks authoritative and tells you nothing about whether to believe it.
The posterior covariance is exactly what separates "the data really determined this" from "the prior guessed this." A parameter with huge posterior variance was not measured — it was assumed. Always ship the uncertainty with the answer.
A second trap: do not confuse a small posterior variance with a correct answer. Cranking up the prior's tightness shrinks the covariance beautifully, but it does so by injecting bias — the ellipse is small because you told it to be, not because the data earned it.
The posterior covariance is not a niche curiosity — it is the quantity a
Watch that ellipse breathe: every time a good measurement arrives (a crisp GPS fix, a landmark the camera recognises), the filter multiplies in a sharp likelihood and the ellipse shrinks. Between measurements, as the vehicle rolls forward on noisy wheels and drifts, the prediction step grows the ellipse again — uncertainty accumulates until the next fix reins it in. That constant shrink-and-grow of the covariance is how an autonomous system stays honest about its own ignorance.
This is the deep lesson of the whole subject: a best guess with no uncertainty is fragile, because you cannot tell a lucky guess from a firm measurement. Quantified uncertainty — the posterior covariance — is what turns a brittle estimate into something you can safely steer a car by.