MilkyWay@home

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User profile Profile Horpah
POLSKA, mieszkam w Czluchowie, moje hobby: literatura science-fiction, astronomia, informatyka. Na zdjeciu moja corka Alicja.
News

PhD Defense Slides
November 19, 2009
I've also linked to the slides from my PhD defense if anyone would like to see them here: [ppt] [keynote]
PPAM 2009 Paper
November 19, 2009
Another update for your reading pleasure. We finished an invited paper for the 2009 Parallel Processing and Applied Mathematics (PPAM) conference about the GPU work here at MilkyWay. We'd like to thank Andreas Przystawik and Dave Anderson for their collaboration on this. Here's a link to the paper: Accelerating the MilkyWay@Home volunteer computing project with GPUs.
PhD Defense
November 19, 2009
Just wanted everyone to know that I successfulled completed my defense today, so I'll have some time to get the server upgraded and all that other great stuff. Hopefully things should be back up and running in the next couple days.
--Travis

Update on Harddrives
November 15, 2009
Just letting everyone know we ordered new hard drives for the server last week, and hopefully they will be here soon. We're hoping to have everything back up and running within the week.
--Travis

An Apology
November 10, 2009
We also really want to apologize for all the recent server issues and lost credit. Hopefully you'll all still be around when we get the server back up and work flowing again. I'll post more as soon as I know about hardware orders and what's going on.
--Travis

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Search Progress

Milkyway@Home uses evolution-inspired search methods to find the optimal fit of models of the Milky Way galaxy to observed star data. By putting models of multiple stripes together we can create a highly accurate three dimensional model of the Milky Way. For each search, the server keeps track of a population of individuals, each corresponding to a possible model of the Milky Way to a stripe of observed stars. The server generates workunits which are combinations of different parent individuals in the population and you calculate the fitness of these child individuals and return the result. When a result is reported to the server that will improve the population, the population is updated and that child individual now becomes a parent. The following figures describe how each search is performing by showing us the best, average, median and worst fitness of each of these populations. The figures are updated every five minutes with your results. By running these evolutionary searches, we can find the best fit of our Milky Way models to the observed data. There is a thread in our forums discussing this in more detail here.





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