Solution

ID: past-exam-of-the-mathematics-course-of-the-university-of-cambridge/2010/iii/paper-37/1/solution

The least-squares estimator minimizes . Differentiation gives , and the full column rank of makes positive definite. Hence
The fitted values are , where the hat matrix is . The regression residuals are . Since is the orthogonal projection matrix onto the column space of , and
This is a singular multivariate normal distribution supported on the -dimensional orthogonal complement of the column space: its components are generally correlated. The equality puts the fitted vector in that column space, while expresses fitted-residual orthogonality. No residual component lies in an explanatory direction that could improve the least-squares fit.
For the calibration model, write for a reading and for the known amount. The first fit assumes with independent errors. Its residual-versus-fitted plot has systematic changes in group means and an increasing within-group spread. These suggest both a nonlinear mean relationship and heteroscedasticity, rather than the random scatter expected from a satisfactory normal linear model.
The Box–Cox transformation plot is a profile log-likelihood for the power parameter . Its maximum is near ; the horizontal line gives an approximate 95% likelihood-ratio confidence interval, which excludes the untransformed value . Since affine rescaling of the response does not change the fitted mean space, fitting the raw power is equivalent to using with an intercept. The second model is
Its residual spread is more even, but observation 17 has a conspicuously negative residual near . This motivates checking for an outlier or recording error. The third fit omits that observation; omission should be justified by that investigation, since choosing exclusions from residuals can affect inference. Some group pattern still remains, so the transformation alone does not certify a perfect model.
At an amount of nanograms, the third fit predicts the transformed mean
Simply applying the inverse power gives . The requested expected reading needs bias correction after an inverse transformation, since for nonlinear . With and , a second-order Taylor expansion gives
Here the correction uses the residual variance, rather than the variance of the estimated fitted mean. The power-transformed Gaussian model is an approximation for positive readings; the fitted mean is over 31 residual standard deviations above zero, so the negative tail has negligible effect on this local approximation. The ordinary inverse-transformed prediction is therefore essentially at the displayed precision.

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