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– architecture and implementation – distributed garbage collection – autonomous migration – split and merge
November 12, 2007 • Carlos Varela
A motivating application in AstroInformatics Programming techniques and patterns
Distributed systems visualization (OverView)
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Carlos Varela
Milky Way Origin and Structure •
Principal Investigators:
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Students:
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Problem Statement:
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How Do Galaxies Form?
H. Newberg (RPI Astronomy), M. Magdon-Ismail, B. Szymanski, C. Varela (RPI CS) N. Cole (RPI Astronomy), T. Desell, J. Doran (RPI CS) What is the structure and origin of the Milky Way galaxy? How to analyze data from 10,000 square degrees of the north galactic cap collected in five optical filters over five years by the Sloan Digital Sky Survey?
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Applications/Implications:
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Approach:
Astrophysics: origins and evolution of our galaxy. Experimental data analysis and simulation To use photometric and spectroscopic data for millions of stars to separate and describe components of the Milky Way
Software:
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Generic Maximum Likelihood Evaluation (GMLE) framework. MilkyWay@Home BOINC project.
Ben Moore, Inst. Of Theo. Phys., Zurich Carlos Varela
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Tidal Streams •
Smaller galaxy gets tidally disrupted by larger galaxy
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Good tracer of galactic potential/dark matter
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Sagittarius Dwarf Galaxy currently being disrupted
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Three other known streams thought to be associated with dwarf galaxies
