... Exploiting the unique broad frequency range and fast-mapping capabilities of the Mopra 22-m telescope, MALT90 will be the first systematic survey of several thousand dense cores in the southern sky at this frequency. ...
... 22-m antennas of the Australia Telescope Compact Array. VLBI data were thus obtained from a series of experiments in March, May, and July 2005. ...
... CASS operates the Australia Telescope National Facility (ATNF), consisting of the Australia Telescope Compact Array (ATCA), the Mopra 22- m telescope, the Parkes 64- m telescope, and the Long Baseline Array (LBA). ...
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Ссылки http://www.atnf.csiro.au/people/bkoribal/LVHIS/NSW13-03277.pdf -- 110.4 Кб -- 19.09.2013 Похожие документы
... 40 60 80 100 Year Number of proposals 1 The AT Compact Array · · · · Formally opened in 1988 Started routine operation in 1990 6 antennas * 22m diameter on E-W track frequency range 1.3 -10 GHz (wavelength range 21 - 3 cm) · angular scales ~ 1 arcsec to ...
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Ссылки http://www.atnf.csiro.au/whats_on/workshops/synthesis2001/material/basics_rpn.pdf -- 1640.4 Кб -- 15.01.2002 Похожие документы
... CO J = 1 0 observations of the Circinus galaxy using the Mopra 22-m radio-telescope . M. Elmouttie, R.F. Haynes, K.L. Jones, PASA, 14 (2), in press. ...
... It is wise to specify a somewhat larger value of 25 m instead of the true antenna diameter of 22m when flagging shadowed data to allow for some safety margin . ...
... 0 C CB cos C B LY C A A@ sin L Z 10 L X 1 Fourier integral got an additional phase term e -2 i(ul+v m) p. 22/28 Advanced tutorial 2 · Image of the 95 GHz methanol maser in G343.12-0.06 following a blind data reduction · But no one should have gone that ...
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Ссылки http://www.atnf.csiro.au/whats_on/workshops/synthesis2008/talks/SIS2008_Voronkov.pdf -- 2887.5 Кб -- 10.10.2008 Похожие документы
... For example, no Si III 1206 · 50 absorption is detected (rest equivalent width W 22m° r NSiIII 1 · 0 в 1012 cm-2 at 4 ) at wavelengths Ao corresponding to the strong Ly absorbers near 1281 ° and 1285 ° Over a range of photoionisation models A A. for (H ...