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    1. De-convolution of a Gaussian beam from planetary observations Bojan Nikolic web
    ... per dimension :param pradius: Radius of planet :param mapsize: Angular size to assign to each map dimension Example: >>> m ... observations. :param pradius: Radius of the planet :param mapsize: Angular size of the map :param ic: Initial condition from ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/oof/beamdeconvolution.html -- 21.3 Кб -- 04.04.2016
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    2. http://www.mrao.cam.ac.uk/yerac/cotter/cotter.ps
    ... Their large angular sizes give excellent opportunities for the study of source physics, and as they lie at the extreme size ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/yerac/cotter/cotter.ps -- 210.0 Кб -- 22.02.1995
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    3. The quasar fraction in a sample of giant radio sources
    ... Their large angular sizes give excellent opportunities for the study of source physics, and as they lie at the extreme size ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/yerac/cotter/cotter.html -- 15.1 Кб -- 08.12.2003
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    4. http://www.mrao.cam.ac.uk/~anthony/latex/Wilkinson.ps
    ... Caltech-Jodrell Bank VLBI Surveys (CJ{300 objects) are sensitive to the angular size range 1.5-50 milliarcsec ( 10 5:5 10 8:5 ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~anthony/latex/Wilkinson.ps -- 28.5 Кб -- 25.06.2000
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    5. High-frequency Radio Continuum Observations of Giant Radio Galaxies
    ... of the six ``classical'' GRGs, i.e. 3C236, 3C326, DA240, NGC6251, NGC315, 4C73.08 which are the largest in angular size ... 3C130, 4C39.04, 4C74.26, 1331-099, 1358+305, 0503-286, 1245+67, 4C34.47, and 8C0821+695, which are smaller in angular size ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/yerac/mack/mack.html -- 17.8 Кб -- 08.12.2003
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    6. VLBI observations of the quasar 3C380
    ... which are unresolved or barely resolved by conventional interferometry (angular size ) and have a steep high frequency spectrum ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/yerac/owsianik/owsianik.html -- 11.9 Кб -- 08.12.2003
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    7. http://www.mrao.cam.ac.uk/yerac/mack/mack.ps
    ... of the six ``classical'' GRGs, i.e. 3C236, 3C326, DA240, NGC6251, NGC315, 4C73.08 which are the largest in angular size ... 3C130, 4C39.04, 4C74.26, 1331­099, 1358+305, 0503­286, 1245+67, 4C34.47, and 8C0821+695, which are smaller in angular size ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/yerac/mack/mack.ps -- 2146.1 Кб -- 22.02.1995
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    8. Galactic SNRs: Documentation
    ... Angular Size of the remnant, in arcminutes, usually taken from the highest ... a single value is quoted for the angular size of the more nearly circular remnants ... in its catalogue entry), although an angular size is still quoted for information ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/projects/surveys/snrs-1996/snrs.info.html -- 30.3 Кб -- 10.04.2016
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    9. http://www.mrao.cam.ac.uk/yerac/owsianik/owsianik.ps
    ... which are unresolved or barely resolved by conventional interferometry (angular size ё 1 0 \Gamma 2 00 ) and have a steep high ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/yerac/owsianik/owsianik.ps -- 164.3 Кб -- 22.02.1995
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    10. Galactic SNRs: Documentation
    ... Angular Size of the remnant, in arcminutes, usually taken from the highest ... a single value is quoted for the angular size of the more nearly circular remnants ... in its catalogue entry), although an angular size is still quoted for information ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/projects/surveys/snrs-1998/snrs.info.html -- 45.6 Кб -- 10.04.2016
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