  The Atacama Large Millimeter/submillimeter Array with the planned electronic
upgrades will deliver an unprecedented amount of deep and high resolution
observations. Wider fields of view are possible with the consequential cost of
image reconstruction. Alternatives to commonly used applications in image
processing have to be sought and tested. Advanced image reconstruction methods
are critical to meet the data requirements needed for operational purposes.
Astrostatistics and astroinformatics techniques are employed. Evidence is given
that these interdisciplinary fields of study applied to synthesis imaging meet
the Big Data challenges and have the potentials to enable new scientific
discoveries in radio astronomy and astrophysics.
