The development of new phased-array systems in radio astronomy, as the low-frequency
array (LOFAR) and the square kilometre array (SKA), formed of a large number of small and …

We describe a flagging and calibration pipeline intended for making quick look images from
GMRT data. The package identifies and flags corrupted visibilities, computes calibration …

We present a novel, general-purpose method for deconvolving and denoizing images from
gridded radio interferometric visibilities using Bayesian inference based on a Gaussian …

We present a new approach to multifrequency synthesis in radio astronomy. Using Bayesian
inference techniques, the new technique estimates the sky brightness and the spectral index …

The Square Kilometre Array (SKA) is a new radio telescope that is currently being designed.
It will consist of two interferometric antenna arrays, one in South Africa and one in Australia …

We describe the development of an FX‐style correlator for very long baseline interferometry
(VLBI), implemented in software and intended to run in multiprocessor computing …

Context. Papers I and II of this series have extended the radio interferometry measurement
equation (RIME) formalism to the full-sky case, and provided a RIME-based description of …

We describe the calibration and imaging heuristics developed and deployed in the Atacama
Large Millimeter/submillimeter Array (ALMA) interferometric data processing pipeline, as of …

The redshifted 21 cm line of neutral hydrogen is a promising probe of the epoch of
reionization (EoR). However, its detection requires a thorough understanding and control of …

Context. Since its formulation by Hamaker et al., the radio interferometer measurement
equation (RIME) has provided a rigorous mathematical basis for the development of novel …