Variations of the antenna primary beam (PB) pattern as a function of time, frequency and polarization form one of the dominant direction-dependent effects at most radio frequency bands. These gains may also vary from antenna to antenna. The A-Projection algorithm, published earlier, accounts for the effects of the narrow-band antenna PB in full polarization. In this paper we present the Wide-Band A-Projection algorithm (WB A-Projection) to include the effects of wide bandwidth in the A-term itself and show that the resulting algo-rithm simultaneously corrects for the time, frequency and polarization dependence of the PB. We discuss the combination of the WB A-Projection and the Multi-term Multi Frequency Synthesis (MT-MFS) algorithm for sim...
Abstract—We consider a troublesome form of non-isoplanatism in synthesis radio telescopes: non-copla...
Modern radio telescopes, such as the Square Kilometre Array (SKA), will probe the radio sky over lar...
The recent demonstration of a real-time direct imaging radio interferometry correlator represents a ...
Aims. We describe MS-MFS, a multi-scale multi-frequency deconvolution algorithm for wide-band synthe...
Abstract. Synthesis imaging in radio astronomy is affected by instrumental and at-mospheric effects ...
© 2015 IEEE. Current and future interferometric imaging arrays in radio astronomy may be limited by ...
22 pages, 6 PostScript figures. Accepted for publication in Astronomy & Astrophysics. Uses aa LaTeX ...
Next-generation radio interferometric telescopes will exhibit non-coplanar baseline configu-rations ...
Current and future interferometric imaging arraysin radio astronomy may be limited by the accuracy w...
Astronomical wide-field imaging of interferometric radio data is computationally expensive, especial...
The required high sensitivities and large fields of view of the new generation of radio in...
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...
The CLEAN algorithm, widely used in radio interferometry for the deconvolution of radio images, perf...
Restricted Access.The Australia Telescope Compact Array and the Very Large Array are currently being...
Abstract—We consider a troublesome form of non-isoplanatism in synthesis radio telescopes: non-copla...
Modern radio telescopes, such as the Square Kilometre Array (SKA), will probe the radio sky over lar...
The recent demonstration of a real-time direct imaging radio interferometry correlator represents a ...
Aims. We describe MS-MFS, a multi-scale multi-frequency deconvolution algorithm for wide-band synthe...
Abstract. Synthesis imaging in radio astronomy is affected by instrumental and at-mospheric effects ...
© 2015 IEEE. Current and future interferometric imaging arrays in radio astronomy may be limited by ...
22 pages, 6 PostScript figures. Accepted for publication in Astronomy & Astrophysics. Uses aa LaTeX ...
Next-generation radio interferometric telescopes will exhibit non-coplanar baseline configu-rations ...
Current and future interferometric imaging arraysin radio astronomy may be limited by the accuracy w...
Astronomical wide-field imaging of interferometric radio data is computationally expensive, especial...
The required high sensitivities and large fields of view of the new generation of radio in...
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...
The CLEAN algorithm, widely used in radio interferometry for the deconvolution of radio images, perf...
Restricted Access.The Australia Telescope Compact Array and the Very Large Array are currently being...
Abstract—We consider a troublesome form of non-isoplanatism in synthesis radio telescopes: non-copla...
Modern radio telescopes, such as the Square Kilometre Array (SKA), will probe the radio sky over lar...
The recent demonstration of a real-time direct imaging radio interferometry correlator represents a ...