Titlebook: Very High Angular Resolution Imaging; Proceedings of the 1 J. G. Robertson,W. J. Tango Conference proceedings 1994 Springer Science+Busines

谆谆教诲

glamor

The SAO Submillimeter Wavelength Arrayith baselines from 9 to 470 m and resolutions as fine as 0‘.‘. Eight receivers will cover all bands from 180 to 900 GHz in linear polarization; two orthogonal polarizations will be available at 350 GHz. Multiyear site testing on Mauna Kea shows that the precipitable water vapor is less than 1 nun fo

迷住

他一致

peptic-ulcer

燕麦

Lunar Occultationsss of astronomical sources: from stellar angular diameters to close binaries, from circumstellar shells to the Galactic Centre..Theresolution and sensitivity offered by lunar occultations still compare favorably withthe capabilities of other more modern methods in the optical and near-infrared. Arem

Tinea-Capitis

Beam Combination for Wide Field Imaginge beam combination method. A beam combination in the pupil plane can completely overcome one of them. In the image plane, a beam combination obeying the rules of geometrical optics can overcome both limitations in principle, but is difficult to achieve in practice. We discuss particularly the real c

OREX

miracle

Source-Noise in Radio Synthesis Images of Polarised Sourcesrms noise at any location in the polarisation images. We compare these results with those for the images of unpolarised sources and discuss the usefulness of deconvolution of snap-shot images in reducing the source-noise from the off-source regions in the images.

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