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

Producing images from interferometer data requires accurate modeling of the sources in the
field of view, which is typically done using the clean algorithm. Given the large number of …

We present a detailed description of the special procedures for calibration and quality
assurance of Atacama Large Millimeter/submillimeter Array (ALMA) observations in Very …

A workstation-based data archive and reduction software system is developed for the
Nobeyama Millimeter Array (NMA). NOVIDAS is used for archiving the output data from the …

New functionality to process Very Long Baseline Interferometry (VLBI) data has been
implemented in the CASA package. This includes two new tasks to handle fringe fitting and …

Abstract CASA, the Common Astronomy Software Applications, is the primary data
processing software for the Atacama Large Millimeter/submillimeter Array (ALMA) and the …

A relational database management system has been implemented on the Caltech millimeter-
wave array for both real-time astronomical and engineering data and post-processing …

The Atacama Large Millimeter/submillimeter Array (ALMA) is a millimeter/submillimeter
(mm/submm) interferometer located in the Atacama desert of northern Chile at an elevation …

We present the design and implementation of an automated data calibration and reduction
pipeline for very long baseline interferometric (VLBI) observations taken at millimeter …

Heterodyne receivers register the sky signal on either a circular polarization basis (where it
is split into left-hand and right-hand circular polarization) or a linear polarization basis …