CYBERSKA
A Cyberinfrastructure platform to meet the needs of data intensive radio astronomy on route to the SKA |
A multiple-beam CLEAN for imaging intra-day variable radio sources
...dely used in radio interferometry for the deconvolution of radio images, performs wel...image) is, to good approximation, a simple convolution between the instrumental poin...ctrum of the sky to become significant. The convolution assumption also breaks down,...3952 days ago
Next -steps in Correction for polarization leakage
...is to the full solution, including the effect of the diffuse total intensity emission, is to use our own Stokes I image as the template for the convolution.2872 days ago
Fundamental Limitations of Pixel Based Image Deconvolution in Radio Astronomy
Deconvolution is essential for radio interferometric imaging to produce scientific quality data because of finite sampling in the Fourier plane. Most deconvolution algorithms are based on CLEAN which uses a grid of image pixels, or clean components. A critical matter in this process is the select...Tags: clean, convolution
4299 days ago