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    41. http://www.mrao.cam.ac.uk/projects/OAS/publications/fulltext/nam04.pdf
    ... Cambridge, UK E. Pedretti, J. D. Monnier University of Michigan, USA COAST UV Coverage 800 600 400 v (10^4 lambda) 200 0 750nm ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/projects/OAS/publications/fulltext/nam04.pdf -- 128.2 Кб -- 20.02.2013
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    42. http://www.mrao.cam.ac.uk/wp-content/uploads/2014/04/GHodosan.pdf
    ... While for example UV, visible or IR molecular emission (as the lightning discharge causes changes in the local chemistry) depends on the composiGon of the atmosphere of the extrasolar body, radio signatures do not have this limitaGon, so they may give us ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/wp-content/uploads/2014/04/GHodosan.pdf -- 1542.0 Кб -- 16.04.2014
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    43. http://www.mrao.cam.ac.uk/projects/aavp/presentations/Koopmans_EoR_SKA1.pdf
    ... UV plane with a relatively uniform (TBD) # of visibilities per UV-annulus is ... UV coverage depends on the filling factor of the core: Max antenna diameter then ... UV coverage and 5o<FoV150MHz<20o for SKA1, one needs 7m < Dant < 30m. This requires ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/projects/aavp/presentations/Koopmans_EoR_SKA1.pdf -- 1801.9 Кб -- 09.12.2010
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    44. http://www.mrao.cam.ac.uk/~dag/UVFLP/ReadMe.txt
    ... UVFLP (to re-order channels in GMRT LSB uv data files within AIPS) ================================================================== To flip the oder of spectral channels in uv databases in AIPS. ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/~dag/UVFLP/ReadMe.txt -- 5.9 Кб -- 08.06.2012
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    45. http://www.mrao.cam.ac.uk/~anthony/latex/Mazzali.ps
    ... Stromlo, Australia The earliest spectrum available of a well-observed, local SN Ia, the UV-optical spectrum of SN 1990N obtained 14 days before B maximum, was modelled with a Monte Carlo code in order to determine its epoch and consequently the rise time ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~anthony/latex/Mazzali.ps -- 26.2 Кб -- 24.06.2000
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    46. http://www.mrao.cam.ac.uk/~bn204/publications/2010/CASASKAJul2010.pdf
    ... Model fitting in UV plane: Good sampling of UV plane reduces the need for this Not much used in present packages/telescopes anyway 4. ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/publications/2010/CASASKAJul2010.pdf -- 199.4 Кб -- 10.08.2012
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    47. Dave Green: research
    ... Some of these bugs applied only to more recent uv datasets written at the GMRT that combine both sidebands into one file, but others apply to single sideband uv datasets also. ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/~dag/my-research.html -- 16.1 Кб -- 29.03.2016
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    48. http://www.mrao.cam.ac.uk/yerac/koester/koester.ps
    ... UV pumping of H 2 so that in the outermost PDR layers, the temperature can increase ... strength of the UV field (10 to 10 6 times the mean UV interstellar radiation field ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/yerac/koester/koester.ps -- 168.3 Кб -- 22.02.1995
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    49. http://www.mrao.cam.ac.uk/~bn204/almasim08/papers/alma_primary_beam_correction_talk.pdf
    ... uv data errors which degrade the image fidelity. -- brightness distribution is ... uv domain. -- for 64 source, image fidelity approaches theoretical noise. -- for 128 ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/almasim08/papers/alma_primary_beam_correction_talk.pdf -- 2607.5 Кб -- 02.12.2008
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    50. http://www.mrao.cam.ac.uk/yerac/mundell/mundell.ps
    ... higher than UV absorption measurements which implies that the optical/UV continuum ... UV lines that the 21­cm absorption, which has a velocity close to systemic and width ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/yerac/mundell/mundell.ps -- 397.3 Кб -- 22.02.1995
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