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    31. http://www.atnf.csiro.au/people/Matthew.Whiting/thesis/ch5.ps.gz
    ... m) F 0:5 good/bad t 0048 097 16.12 3.61 Combined { 0.15 0.97 good 1110 217 24.41 7.67 Combined { 1.85 0.88 good 1156 094 21.95 ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/Matthew.Whiting/thesis/ch5.ps.gz -- 170.7 Кб -- 29.03.2006
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    32. http://www.atnf.csiro.au/vlbi/dokuwiki/lib/exe/fetch.php/difx/meetings/sydney2012/anderson_space_vlbi.pdf
    ... DiFX Annual Meeting, Sydney, 2012 Sep 24 James M Anderson 13/21 Comparison Against ASC Correlator Report from Michael Bietenholz (u,v,w) differences of about 0.3% for ground­ spacecraft and ground­ground baselines EF­JB baseline shows 180 degree phase ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/vlbi/dokuwiki/lib/exe/fetch.php/difx/meetings/sydney2012/anderson_space_vlbi.pdf -- 743.4 Кб -- 24.09.2012
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    33. http://www.atnf.csiro.au/management/atuc/2006jun/docs/3.4_Tid.pdf
    ... To test this, observ ations at 13 c m have been made to map the beam and results appear promising. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/management/atuc/2006jun/docs/3.4_Tid.pdf -- 101.7 Кб -- 02.06.2006
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    34. Introduction
    ... The CCD detector consists of two arrays of pixels with each array containing 2048 elements; each pixel is 13 m wide by 750 m high. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/14_3/marsden/paper/node1.html -- 52.0 Кб -- 08.04.2016
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    35. http://www.atnf.csiro.au/people/Matthew.Whiting/thesis/ch5.pdf
    ... 7.13 > 5.39 6.22 6.54 6.27 Best fit model Combined Combined Combined Combined Power law Power law Combined Power law Combined ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/Matthew.Whiting/thesis/ch5.pdf -- 447.4 Кб -- 29.03.2006
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    36. Polarimetry
    ... A CdS waveplate is used for 8 - 13 m observations, and a CdSe waveplate is used at 20 m. The waveplate is mounted outside the cryostat above the dichroic mirror, and is is rotated to four positions in the beam (corresponding to position angle rotations of ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/14_2/smith/paper/node4.html -- 57.0 Кб -- 08.04.2016
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    37. http://www.atnf.csiro.au/projects/askap/newdocs/Abstract_NTD_Receiver.pdf
    ... A total of 24 down-converters are required to take the signals from the LNAs located with the array of feeds at the focal plane of a 13.7 m diameter parabolic dish reflector antenna. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/projects/askap/newdocs/Abstract_NTD_Receiver.pdf -- 15.9 Кб -- 09.02.2006
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    38. NIMPOL: An imaging polarimeter for the mid-infrared.
    ... D.Aitken@roe.ac.uk . We have built an imaging polarimeter for use at mid-infrared wavelengths ( i.e. N band or 8 - 13 m). ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/14_2/smith/paper/index.html -- 52.2 Кб -- 08.04.2016
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    39. http://www.atnf.csiro.au/projects/askap/newdocs/Abstract_NTD_Interferometer.pdf
    ... outlines an experiment currently being prepared for the NTD, and relies on the installation of two recently refurbished 13.7 m diameter antennas which will be fitted with various feed technologies resulting from CSIRO's research program into Focal Plane ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/projects/askap/newdocs/Abstract_NTD_Interferometer.pdf -- 16.5 Кб -- 09.02.2006
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    40. http://www.atnf.csiro.au/management/atuc/2006jun/docs/6_NTD.pdf
    ... The development of the 2-element interferometer (using 2 refurbished 13.7 m antennas from ex-Fleurs) being used at Marsfield for the above-mentioned FPA work is progressing as planned. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/management/atuc/2006jun/docs/6_NTD.pdf -- 83.3 Кб -- 05.06.2006
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