Gaussian process-based Bayesian imaging of bolometric (sub-)millimetre data
Widefield single-dish telescopes operating at (sub-)mm wavelengths ($\lambda \sim 4$~mm to 350~$\mu$m) tend to feature much faster mapping speeds than radio interferometers at the same wavelengths, and are more suitable for measuring signals on larger spatial scales. However, the data are dominated by atmospheric fluct...