... The A LL OB option is valid only for uv -coverage plots, where it implies that the data of all output beams, channels, and baselines shall be plotted. ...
... it correlates the dirty map (i.e. the Fourier transform of the visibility data) with the dirty beam (i.e. the Fourier transform of the uv coverage) and place a so-called CLEAN component (i.e. delta function type pixel) where it found a maximum correlation ...
... Active Galactic Nuclei (AGN) are being discovered in ever-larger numbers over the whole electromagnetic spectrum (radio, infrared, optical/UV, X-ray and нЕ-ray), providing different windows on AGN physics. ...
... star clusters in Fornax', 'dynamical sub-structures in the star cluster and satellite systems in Fornax', 'the multi-colour (UV to NIR) view of stellar populations in Fornax galaxies', 'constraining the dark matter distribution in the Fornax cluster', etc ...
... powers" up to 80,000 in the UV-blue spectral region and 115,000 in the red region [3 ... that produce faint absorption lines in the extreme blue and UV part of the spectrum ...
... powers" up to 80,000 in the UV-blue spectral region and 115,000 in the red region [3 ... that produce faint absorption lines in the extreme blue and UV part of the spectrum ...
... powers" up to 80,000 in the UV-blue spectral region and 115,000 in the red region [3 ... that produce faint absorption lines in the extreme blue and UV part of the spectrum ...