... For HD 93129B and HD 93128 we derive 3 upper limits of _ M < (f T ) 3=4 2:13 10 5 M yr 1 . ... 5 M yr 1 for HD 93129A and 3 upper limits of (f T ) 3=4 2:13 10 5 M yr 1 for HD 93129B and HD 93128, where fT is the thermal ...
... resolved x-ray spectra have determined the form of the dark matter potential over the mass scale from 10^13-3x10^15 M. Comparison of lensing, optical,x-ray and Sunyzev-Zeldovich observations have allowed robust tests of the general scenario of structure ...
... 13 3 of 13 4 of 13 5 of 13 6 of 13 7 of 13 8 of 13 9 of 13 10 of 13 11 of 13 12 of 1313 of 13 Drawn By MMMMMMMMMMMMM Leach Leach Leach Leach Leach Leach Leach Leach Leach Leach Leach Leach Leach Ateg2:\usr2\users\mbeam\s6\elec\xilinx\3levprog ...
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Ссылки http://www.atnf.csiro.au/research/electronics/docs/mb/sampler.pdf -- 56.9 Кб -- 07.04.1998 Похожие документы
... Note that signal o#sets in RA are 00:00:02 (30''), and reference o#sets in RA are 00:02:00 (30 m ) (see §13, p43). $ unit 1 raj = 18:18:55.34 ! ...
... Using the novel 13-beam receiver system on the 64-m Parkes Telescope, Ekers et al. searched for flashes of radio wave lasting just a nanosecond, generated by neutrinos interacting with rocks under the moon's surface (known as the Askaryan effect). ...
... Therefore, arrangements were made with Sydney University to acquire two disused 13.7 m parabolic dishes, complete with mounts, from the old Fleurs observatory. ...
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Ссылки http://www.atnf.csiro.au/projects/mnrf2001/Astronomy_MNRF_0405.pdf -- 1465.7 Кб -- 13.10.2005 Похожие документы
... 13 Forward Selection resulting features: dered ( z psf )- dered ( i petrosian dered ( g psf )- dered ( r model dered ( r psf )- dered ( z model dered ( r dered ( z model u psf - g petrosian ) z psf - i petrosian ) g psf - r model ) r psf - z model +r ) r ...
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Ссылки http://www.atnf.csiro.au/research/workshops/2013/astroinformatics/talks/polsterer.pdf -- 526.2 Кб -- 13.12.2013 Похожие документы