A general framework is presented for modeling direction-dependent effects that are also baseline-dependent, as part of the calibration and imaging process. Within this framework such effects are represented as a parametric linear model in which basis functions account for direction dependence, whereas expansion coefficients account for the baseline dependence. This separation enables the use of a multiple fast Fourier transform-based implementation of the forward calculation (sky to visibility) in a manner similar to the W-stacking solution for non-coplanar baselines, and offers a potential improvement in computational efficiency in scenarios where the gridding operation in a convolution-based approach to direction-dependent effects may be ...
Context. Since its formulation by Hamaker et al., the radio interferometer measurement equ...
Next-generation radio interferometric telescopes will exhibit non-coplanar baseline configurations a...
International audienceTraditional radio interferometric correlators produce regular-gridded samples ...
© 2015 ESO. A general framework is presented for modeling direction-dependent effects that are also ...
A general framework is presented for modeling direction-dependent effects that are also baseline-dep...
Current and future interferometric imaging arraysin radio astronomy may be limited by the accuracy w...
© 2015 IEEE. Current and future interferometric imaging arrays in radio astronomy may be limited by ...
Direction dependent effects can be classified as known/measured effects (which need not be solved fo...
Reproduced with permission from Astronomy & Astrophysics, © 2018 ESO. Content in the UH Research Arc...
Calibration in radio interferometry describes the process of estimating and correcting for instrumen...
In radio astronomy obtaining a high dynamic range in synthesis imaging of wide fields requires a cor...
Thesis (MEng)--Stellenbosch University, 2017.ENGLISH ABSTRACT: This thesis presents the implementati...
In radio interferometry, observed visibilities are intrinsically sampled at some interval in time an...
The standard wide-field imaging technique, the w-projection, allows correction for wide fields of vi...
The paper reviews progress in imaging in radio interferometry for the period 1993-1996. Unlike an op...
Context. Since its formulation by Hamaker et al., the radio interferometer measurement equ...
Next-generation radio interferometric telescopes will exhibit non-coplanar baseline configurations a...
International audienceTraditional radio interferometric correlators produce regular-gridded samples ...
© 2015 ESO. A general framework is presented for modeling direction-dependent effects that are also ...
A general framework is presented for modeling direction-dependent effects that are also baseline-dep...
Current and future interferometric imaging arraysin radio astronomy may be limited by the accuracy w...
© 2015 IEEE. Current and future interferometric imaging arrays in radio astronomy may be limited by ...
Direction dependent effects can be classified as known/measured effects (which need not be solved fo...
Reproduced with permission from Astronomy & Astrophysics, © 2018 ESO. Content in the UH Research Arc...
Calibration in radio interferometry describes the process of estimating and correcting for instrumen...
In radio astronomy obtaining a high dynamic range in synthesis imaging of wide fields requires a cor...
Thesis (MEng)--Stellenbosch University, 2017.ENGLISH ABSTRACT: This thesis presents the implementati...
In radio interferometry, observed visibilities are intrinsically sampled at some interval in time an...
The standard wide-field imaging technique, the w-projection, allows correction for wide fields of vi...
The paper reviews progress in imaging in radio interferometry for the period 1993-1996. Unlike an op...
Context. Since its formulation by Hamaker et al., the radio interferometer measurement equ...
Next-generation radio interferometric telescopes will exhibit non-coplanar baseline configurations a...
International audienceTraditional radio interferometric correlators produce regular-gridded samples ...