For distinct sibling supernovae and in the same galaxy, the shared fluctuation is the only common random term. Independence and linearity of covariance therefore give
Their correlation coefficient is
This is the intraclass correlation coefficient of the galaxy-level random intercept model.
Write the Cepheid measurement as , where , and define the calibrated absolute magnitude data
Thus has a multivariate normal distribution with mean and covariance matrix
The Hubble law and the definition of distance modulus give
Consequently, with
the Hubble-flow observations are independent random variables satisfying . Apart from a factor independent of the parameters, the joint likelihood function is
The expression extends by continuity to a singular limiting covariance such as .
Let
and set
The within-galaxy contrasts contain no , so the parameter-dependent log-likelihood reduces to
The score equations give the maximum-likelihood estimators
The calibrator and Hubble-flow samples are independent, so both estimators are unbiased and
The Fisher information matrix for is
Hence : attains the multiparameter Cramer-Rao bound.
The invariance property of maximum likelihood estimation gives
Since , the ratio has a log-normal distribution. Its exact variance is
and the lowest-order delta method approximation is
For fixed , case (i) has , whereas case (ii) has . Because and is the same in both cases, independent supernova-level variation in case (ii) gives the smaller fractional variance: averaging reduces it, while a shared galaxy fluctuation does not average away.

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