... Each 15 m pixel corresponds to 20.''63 on the sky, giving a total field size of square. The H filter was centered at 6569 ц…\ with a FWHM of 15 ц…. ...
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Ссылки http://www.atnf.csiro.au/people/Amy.Kimball/Publications/norris_et_al_2011.pdf -- 1420.2 Кб -- 02.10.2013 Похожие документы
... 0 -50 -50 -100 -100 -50 0 Mpc/h 50 100 -100 -100 100 -50 0 Mpc/h 50 100 50 0 -50 Figure 6: Here mock catalogues are separated in two phases: the halo catalogue (M 1.62 в 1012M) and the background field (M < 1.62 в 1012M) representing 63% of the total mass ...
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Ссылки http://www.atnf.csiro.au/research/LVmeeting/posters/GLavaux-poster.pdf -- 1313.3 Кб -- 02.07.2007 Похожие документы
... Sources and Data Mean (µm) 0.440 0.550 0.700 0.880 1.239 1.649 2.192 Zero magnitude flux (F , W m-2 µm-1 ) 6.32 в 10-8 3.63 в 10-8 2.18 в 10-8 1.13 в 10-8 3.11 в 10-9 1.15 в 10-9 4.10 в 10-10 Table 4.1: Assumed fluxes of a star with zero magnitude, for ...
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Ссылки http://www.atnf.csiro.au/people/Matthew.Whiting/thesis/ch4.pdf -- 133.0 Кб -- 29.03.2006 Похожие документы
... Hartley, M., Manchester, R. N., Smith, R. M., Tritton, S. B., & Goss, W. M. 1986, A&AS, 63, 27 Kramer, C., Zimmermann, T., Stutzki, J., & Winnewisser, G. 1993, in The Physics and Chemistry of Interstellar Molecular Clouds, ed. G. Winnewisser & G. Pelz ...
... In other words, 63% of the antennas should be inside the diameter D, and the remaining 37% outside that diameter Figure 2 shows the resulting value of p for the two cases, m=1 and m=2, as a function of n. 2 12/04/00 Figure 2: The consequent proportions of ...
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Ссылки http://www.atnf.csiro.au/projects/askap/techdocs/Constraints_on_SKA_array_configurations.pdf -- 29.5 Кб -- 12.04.2000 Похожие документы