A p-bit array runs thousands of chains at once, each only a few sweeps long, and it needs a rule for when to stop. The standard rule, R-hat, asks whether chains started in different places have come to agree, and it was built for a few long chains. Nested R-hat, from Margossian, Gelman and colleagues in 2024, was built for the many-short-chains regime. It groups chains into superchains that share a starting point and watches how much the superchains still disagree, which the authors call the nonstationary variance, and so, by proxy, the squared bias. Every part of it can be computed exactly from the machine's one-step law, with no chain run at all, and that exactness shows where the proxy holds and where it does not. From starting points spread across the space it holds: on ten-spin glasses, when the rule first passes, the squared bias is at most half the tolerance. Three things it cannot see. A start every superchain shares, such as a cleared register, leaves nothing to disagree about, so the statistic sits exactly at its floor from the first sweep and passes on an answer that has not moved. A bias every start shares, which a cold ferromagnet's energy has, passes three tolerances early. And a machine that converges to the wrong law, as a synchronous sweep does, passes as soon as it has converged, with its energy here nine standard deviations from the Boltzmann value. A convergence check certifies that the machine has settled, into whatever it settles into. Whether that is the distribution you asked for is a second question, and it needs a second measurement.