For distinct sibling supernovae and in the same galaxy, the shared fluctuation is the only common random term. Independence and linearity of covariance therefore giveTheir correlation coefficient isThis is the intraclass correlation coefficient of the galaxy-level random intercept model.
Write the Cepheid measurement as , where , and define the calibrated absolute magnitude dataThus has a multivariate normal distribution with mean and covariance matrix
The Hubble law and the definition of distance modulus giveConsequently, withthe Hubble-flow observations are independent random variables satisfying . Apart from a factor independent of the parameters, the joint likelihood function isThe expression extends by continuity to a singular limiting covariance such as .
Letand setThe within-galaxy contrasts contain no , so the parameter-dependent log-likelihood reduces toThe score equations give the maximum-likelihood estimatorsThe calibrator and Hubble-flow samples are independent, so both estimators are unbiased andThe Fisher information matrix for isHence : attains the multiparameter Cramer-Rao bound.
The invariance property of maximum likelihood estimation givesSince , the ratio has a log-normal distribution. Its exact variance isand the lowest-order delta method approximation isFor 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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