Stack the observations as and set
Let and denote matrices obtained by evaluating the two Gaussian process covariance kernels. Independence of the quasar light curve, gravitational microlensing, and Gaussian noise processes gives
where . Thus is a multivariate normal distribution and its Gaussian-process marginal likelihood is
The off-diagonal blocks are essential: both images contain the same delayed Ornstein-Uhlenbeck process.
At the fitted parameters, let and . For prediction times define
The microlensing processes and measurement errors contribute no cross-covariance with the latent quasar light curve. The Gaussian process regression posterior is therefore
The requested pointwise posterior variances are the diagonal entries of the latter matrix.
Use broad proper uniform priors for , , and over physically plausible ranges, and broad log-uniform priors for the positive scales and . Then
A Random-walk Metropolis algorithm can update with a multivariate Gaussian proposal distribution. Initialize several dispersed chains near plausible cross-correlation delays and near the marginal-likelihood optimum; reject proposals outside the prior bounds; discard warm-up while adapting only the proposal scale and covariance; then freeze the kernel and retain a long run. Evaluate trace plots, autocorrelations, acceptance rates, between-chain agreement, and the effective sample size of a Markov chain. Posterior predictive quasar light curves provide a model check.
Write the target posterior density as and the proposal distribution density as . The Metropolis–Hastings algorithm accepts a proposed move with
For distinct states,
which is symmetric in and . The rejection probability supplies the diagonal part, so the entire transition kernel satisfies detailed balance. Integrating the detailed-balance identity over the starting state proves . Hence the posterior is a stationary distribution; an irreducible Markov chain that is also an aperiodic Markov chain converges uniquely to it.

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