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    21. http://www.atnf.csiro.au/people/Ray.Norris/papers/n296.pdf
    ... The broad frequency coverage coupled with the compact, hybrid configurations (with baselines as short as 31 m) make the ATCA an excellent instrument to detect molecular gas at high-redshifts. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/Ray.Norris/papers/n296.pdf -- 385.2 Кб -- 28.10.2012
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    22. PM Survey Publications
    ... F., D'AMICO, N., POSSENTI, A., KASPI, V.M., STAIRS, I.H. " Young Pulsars from the Parkes Multibeam Pulsar Survey and their Associations" , Neutron Stars in Supernova Remnants (ASP Conference Proceedings), eds P.O.Slane and B.M.Gaensler,271, 31-36 (2002 ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/pulsar/pmsurv/papers.html -- 23.4 Кб -- 02.10.2012
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    23. http://www.atnf.csiro.au/people/rnorris/N197.pdf
    ... The shortest baseline was 31 m, and the longest 6000 m. Table 2 summarises the observations, and Figure 1 shows the pointing ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/rnorris/N197.pdf -- 2134.8 Кб -- 14.04.2005
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    24. Evolutionary Paths in Galaxy Morphology
    ... Now, striking new evidence discovered in M 31 and NGC 3379 suggests that the metal-poor outermost halo can be isolated at very large radii, R > 12Reff. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/research/conferences/2013/gzo/abstracts/a92.html -- 49.1 Кб -- 11.04.2016
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    25. http://www.atnf.csiro.au/projects/askap/techdocs/GPS_Int_Explain.pdf
    ... NTIA, October 1994, JTIDS EMC Features Guidelines, SPS WG-1 TR-91-001 Revision A. Leiter, M., 31 March 1998, "The Ratio of Peak-to-RMS Noise Power in the IFF Notches," MITRE Memorandum D620-M-008, The MITRE Corporation, Bedford, Massachusetts. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/projects/askap/techdocs/GPS_Int_Explain.pdf -- 371.8 Кб -- 09.12.1999
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    26. ATNF Publications 2008
    ... Published . *WESTMEIER, T., BRAUN, R., BRUNS, C., KERP, J. & THILKER, D.A. "The relics of structure formation: high-velocity clouds around M 31". ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/research/publications/AT2008.html -- 96.7 Кб -- 08.04.2016
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    27. http://www.atnf.csiro.au/the_atnf/annual_reports/2002/17189_p17-37.pdf
    ... Scl in several compact configurations of three antennas, with baselines ranging from 31 ­ 413 m, between June and October 2002 ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/the_atnf/annual_reports/2002/17189_p17-37.pdf -- 1956.0 Кб -- 14.07.2003
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    28. ATNF Science Highlights 2002
    ... We observed R Scl in several compact configurations of three antennas, with baselines ranging from 31-413 m, between June and October 2002. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/research/highlights/2002/wong/wong.html -- 50.9 Кб -- 08.04.2016
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    29. http://www.atnf.csiro.au/iau-comm31/pdf/circular06.pdf
    ... Here are some informations or events related to our Commission 1)Election of officers for the triennium 2003-2006 For 2003-2006, the present vice-president D.N. Matsakis will be president of C om m i s s i on 31. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/iau-comm31/pdf/circular06.pdf -- 8.1 Кб -- 24.09.2008
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    30. http://www.atnf.csiro.au/observers/memos/AT40.3.1_102.pdf
    ... torque of 256 T-m X Rotating mass = 800 T X = 31 cm. 9.5 m Locus of the counterweight centre of mass Figure 2: A geometrical ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/observers/memos/AT40.3.1_102.pdf -- 57.2 Кб -- 16.04.2015
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