... Simfest Day 1 wrap-up Lister Staveley-Smith (ICRAR/UWA) Millennium/VIMOS simulation 1 TOOLS AND METHODS > Dark matter simulations (Chris Power, Greg Poole) - Precision model for underlying dark halo distribution - Possible to simulate large volumes with ...
[
Текст
]
Ссылки http://www.atnf.csiro.au/research/WALLABY/Wallaby2011/SIM-FEST2011-LSS.pdf -- 348.8 Кб -- 01.12.2011 Похожие документы
... ST (Single Thread) · SMT (Simultaneous Multi-Threading) Benchmark data set: Millennium II simulation output containing about 10 billion particles Splotch: benchmark results Millennium run Total wallclock time minus read time Millenium II simulation Read ...
[
Текст
]
Ссылки http://www.atnf.csiro.au/research/WALLABY/Wallaby2011/SIM-FEST2011-KDolag2.pdf -- 1643.7 Кб -- 07.12.2011 Похожие документы
... the proceedings of the conference "Astronomy Education For the Next Millennium", held in Kingswood, Sydney in July 1999 ... PDF (45.5 kb) . Preparing Astronomy Majors for the Job Market of the New Millennium . Victor Migenes. ...
... 2000, 17, 145148 Preparing Astronomy Majors for the Job Market of the New Millennium Victor Migenes Department of Astronomy, University of Guanajuato, Apdo Postal 144, Guanajuato, GTO, CP 36000, Mexico vmigenes@astro.ugto.mx Received 1999 September 1 ...
... Using redshifts from the Millennium Galaxy Catalogue (MGC) combined with imaging data from the Sloan Digital Sky Survey (SDSS) and the UK Infrared Deep Sky Survey (UKIDSS) we have now reconstructed the coarse energy spectrum over the full optical/near-IR ...
... I would also like to thank Professor Julietta Fierro for inviting me to attend the Astronomy Education in the New Millennium conference, and the IAU and SAAO for funding. ...
... Predicting GW signals: We have used the millennium simulations and accompanying semi-analytic models to predict the strength and non-Gaussianity of the gravitational wave background from massive black hole binaries (Ravi et al. ...
... of particular interest to us here as such events are the primary interest of the Pierre Auger observatory which will begin operations early in the new millennium and will have a collecting area of 3000 km 2 at each of a southern and a northern location ...