Stars orbiting the compact radio source Sgr A* in the Galactic Center serve as precision
probes of the gravitational field around the closest massive black hole. In addition to …

Several physical problems require Bayesian inference of spatial, or spatio-temporal
phenomenon–often modeled as random fields defined on a continuous domain–from a …

Next-generation radio interferometers like the Square Kilometer Array have the potential to
unlock scientific discoveries thanks to their unprecedented angular resolution and …

Stellar orbits at the Galactic Center provide a very clean probe of the gravitational potential
of the supermassive black hole. They can be studied with unique precision, beyond the …

Modern interferometers routinely provide radio-astronomical images down to subarcsecond
resolution. However, interferometers filter out spatial scales larger than those sampled by …

Context. Imaging in radioastronomy is an ill-posed inverse problem. However, with
increasing sensitivity and capabilities of telescopes, several strategies have been …

Context. Self-calibration methods with the CLEAN algorithm have been widely employed in
very long baseline interferometry (VLBI) data processing in order to correct antenna-based …

Context. Very long baseline interferometry (VLBI) is a radio-astronomical technique whereby
the correlated signal from various baselines is combined into an image of the highest …

Strong-lensing images provide a wealth of information both about the magnified source and
about the dark matter distribution in the lens. Precision analyses of these images can be …

Efficiently accessing the information contained in non-linear and high dimensional
probability distributions remains a core challenge in modern statistics. Traditionally …