Solution

ID: past-exam-of-the-mathematics-course-of-the-university-of-cambridge/2022/iii/paper-219/1/c/solution

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.

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