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CYBERSKA
A Cyberinfrastructure platform to meet the needs of data intensive radio astronomy on route to the SKA |
Results for "media"
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AGN Obscuration and the Unified Model
...g the need for a more complex geometrical distribution of the absorbing media. In this paper we review the various pieces of evidence for obscuring media on different scales, from the...3791 days ago
Modeling the polarization of radio-quiet AGN from the optical to the X-ray band
...broad-band continuum source that is surrounded by several reprocessing media with different geometries and...om the complex radiative coupling between different, axis-symmetric AGN media. Using the latest version of...3706 days ago
- ...spersive terms. We call this method source-frequency phase referencing. Provided that the switching cycles match the properties of the propagation media, one can recover the source a...
4104 days ago
Optimal wavelength for radio polarization observations
...range of objects. Methods. The optimum wavelength of maximum polarized intensity (PI) is computed for the cases of depolarization in magneto-ionic media including regular magnetic fi...4152 days ago
Comparison of RFI Mitigation Strategies for Dispersed Pulse Detection
Impulsive radio-frequency signals from astronomical sources are dispersed by the frequency dependent index of refraction of the interstellar media and so appear as chirped signals wh...3792 days ago
The evolution of the large-scale emission in Fanaroff–Riley type I jets
...mall flux variations with time. The shocked jet synchrotron emission would dominate the X-ray band, although the shocked interstellar/intracluster media thermal component alone may b...4160 days ago
