Fourier Plane Image Combination by Feathering
arXiv:1707.02272 · doi:10.1088/1538-3873/aa793f
Abstract
Astronomical objects frequently exhibit structure over a wide range of scales whereas many telescopes, especially interferometer arrays, only sample a limited range of spatial scales. In order to properly image these objects, images from a set of instruments covering the range of scales may be needed. These images then must be combined in a manner to recover all spatial scales. This paper describes the feathering technique for image combination in the Fourier transform plane. Implementations in several packages are discussed and example combinations of single dish and interferometric observations of both simulated and celestial radio emission are given.
7 pages, 4 figures
References in corpus (4)
- A 20cm Survey of the Galactic Center Region I: Detection of Numerous Linear Filaments
- A Wide-area VLA Continuum Survey near the Galactic Center at 6 and 20 cm Wavelengths
- GBT Multiwavelength Survey of the Galactic Center Region
- Revisiting the radio interferometer measurement equation. III. Addressing direction-dependent effects in 21 cm WSRT observations of 3C 147
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