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1 posted on 06/01/2005 9:55:10 PM PDT by Ernest_at_the_Beach
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2 posted on 06/01/2005 9:57:28 PM PDT by Ernest_at_the_Beach (This tagline no longer operative....floated away in the flood of 2005 ,)
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To: KevinDavis

fyi


4 posted on 06/01/2005 10:03:12 PM PDT by Ernest_at_the_Beach (This tagline no longer operative....floated away in the flood of 2005 ,)
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To: Ernest_at_the_Beach

Looks just a smidge like "Collusus, The Forbin project." bump, bttt.


5 posted on 06/01/2005 10:03:12 PM PDT by Not now, Not ever! (This tagline is temporarily closed for re-modeling)
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To: Ernest_at_the_Beach; All
Cool (Free!) Astronomy-related Software:
Please FReepmail other suggestions
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    Outlines, boundaries, and names of constellations can be displayed, as well as names and Bayer/Flamsteed designations of stars brighter than a given threshold. A database of more than 500 deep-sky objects, including all the Messier objects and bright NGC objects can be plotted to a given magnitude. The ecliptic and celestial equator can be plotted, complete with co-ordinates.
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6 posted on 06/01/2005 10:10:05 PM PDT by martin_fierro (Chat is my milieu)
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To: Ernest_at_the_Beach
I can't be sure, but from the URL on that supercomputer picture, which ends in the string "superc_wildcat_203.jpg", I suspect that is a BBC stock photo of a supercomputer, that happens to be a Sun Wildcat, which was not the computer used for this research.

The system used for this research is the principal supercomputer at the Max Planck Society's Supercomputing Centre in Garching, Germany, the Regatta, as described at http://www.rzg.mpg.de/computing/IBM_P/hardware.html:


The IBM pSeries Supercomputer

The pSeries "Regatta" system is based on Power 4 processor technology.
Node characteristics are:
32-way "Regatta" compute nodes (eServer p690), equipped with 1.3 GHz Power 4 processors, with a peak perf. of 166 GFlop/s and 64 GB of main memory per node.

Since Oct 2001, an 8 proc test system had been installed.

From January 2002, a six node system with an aggregated performance of 1 TFlop/s and 1/2 TB of main memory has been in operation.

In mid 2002, the system has been extended to 22 compute nodes and 2 I/O nodes with an aggregated peak performance of 3.8 TFlop/s and 1.8 TB of main memory.

In Jan/Feb 2003, the system was moved to the new computer building with significantly increased disk space.

After initial tests with the new IBM High Performance Switch (HPS, "Federation Switch") as of early Sep 2003, the system was upgraded to this fast node interconnect technology in December 2003, together with a system expansion to 4.2 TF peak performance.

There are now 25 compute nodes and 2 I/O nodes, connected by the High Performance ("Federation") Switch, with four links per Regatta node.


The Max Planck Institute press release for this Nature article: Supercomputer Simulations explain the Formation of Galaxies and Quasars in the Universe explains quite a bit more about this work.

Here's the cover of the Nature magazine with the article:


Nature - 2 June 2005.
And here is one of the several impressive images linked off the above press release:

8 posted on 06/02/2005 12:33:41 AM PDT by ThePythonicCow (To err is human; to moo is bovine.)
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