Abstract—We consider a troublesome form of non-isoplanatism in synthesis radio telescopes: non-coplanar baselines. We present a novel interpretation of the non-coplanar baselines effect as being due to differential Fresnel diffraction in the neighborhood of the array antennas. We have developed a new algorithm to deal with this ef-fect. Our new algorithm, which we call “W-projection”, has markedly superior performance compared to existing algorithms. At roughly equivalent levels of accuracy, W-projection can be up to an order of magnitude faster than the corresponding facet-based algorithms. Furthermore, the precision of result is not tightly coupled to computing time. W-projection has important consequences for the design and operation of ...
A detailed investigation of projection e†ects involved in the study of classical double sources is p...
This study investigates some of the consequences of representing the sky by a rectangular grid of pi...
The problem of image reconstruction in radio interferometry is traditionally solved through the appl...
Next-generation radio interferometric telescopes will exhibit non-coplanar baseline configu-rations ...
The standard wide-field imaging technique, the w-projection, allows correction for wide fields of vi...
Astronomical wide-field imaging of interferometric radio data is computationally expensive, especial...
Astronomical wide-field imaging of interferometric radio data is computationally expensive, especial...
Imaging in radio astronomy entails the Fourier inversion of the relation between the sampled spatial...
Variations of the antenna primary beam (PB) pattern as a function of time, frequency and polarizatio...
Sky curvature and non-coplanar effects, caused by low frequencies, long baselines, or small aperture...
Modern radio telescopes, such as the Square Kilometre Array (SKA), will probe the radio sky over lar...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society....
Radio telescopes with baselines that span thousands of kilometres and with fields of view that span ...
© 2017 ESO. Radio telescopes with baselines that span thousands of kilometres and with fields of vie...
A general framework is presented for modeling direction-dependent effects that are also baseline-dep...
A detailed investigation of projection e†ects involved in the study of classical double sources is p...
This study investigates some of the consequences of representing the sky by a rectangular grid of pi...
The problem of image reconstruction in radio interferometry is traditionally solved through the appl...
Next-generation radio interferometric telescopes will exhibit non-coplanar baseline configu-rations ...
The standard wide-field imaging technique, the w-projection, allows correction for wide fields of vi...
Astronomical wide-field imaging of interferometric radio data is computationally expensive, especial...
Astronomical wide-field imaging of interferometric radio data is computationally expensive, especial...
Imaging in radio astronomy entails the Fourier inversion of the relation between the sampled spatial...
Variations of the antenna primary beam (PB) pattern as a function of time, frequency and polarizatio...
Sky curvature and non-coplanar effects, caused by low frequencies, long baselines, or small aperture...
Modern radio telescopes, such as the Square Kilometre Array (SKA), will probe the radio sky over lar...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society....
Radio telescopes with baselines that span thousands of kilometres and with fields of view that span ...
© 2017 ESO. Radio telescopes with baselines that span thousands of kilometres and with fields of vie...
A general framework is presented for modeling direction-dependent effects that are also baseline-dep...
A detailed investigation of projection e†ects involved in the study of classical double sources is p...
This study investigates some of the consequences of representing the sky by a rectangular grid of pi...
The problem of image reconstruction in radio interferometry is traditionally solved through the appl...