Milkyway@Home uses the BOINC platform to harness volunteered computing resources, creating a highly accurate three dimensional model of the Milky Way galaxy using data gathered by the Sloan Digital Sky Survey. This project enables research in both astroinformatics and computer science.
In computer science, the project is investigating different optimization methods which are resilient to the fault-prone, heterogeneous and asynchronous nature of Internet computing; such as evolutionary and genetic algorithms, as well as asynchronous newton methods. While in astroinformatics, Milkyway@Home is generating highly accurate three dimensional models of the Sagittarius stream, which provides knowledge about how the Milky Way galaxy was formed and how tidal tails are created when galaxies merge.
Milkyway@Home is a joint effort between Rensselaer Polytechnic Institute's departments of Computer Science and Physics, Applied Physics and Astronomy. Feel free to contact us via our forums, or email astro[at]cs.lists.rpi[dot]edu.
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Milkway@home is funded through a grant from the National Science Foundation (NSF). Any opinions, findings, and conclusions or recommendtions expressed in this material are those of the author(s) and do not necessarily reflect the views of the NSF.
Individual grants are listed on the information page.
MilkyWay@home is currently experiencing an outage for the Separation Validator. I brought it back up once, and then it crashed again. I am trying to bring it back up. In the meantime, connections to the download/upload servers may stop and start intermittently as I work on the server.
Thanks for your patience, I will keep you updated as things change.
21 Sep 2021, 16:13:00 UTC · Discuss
NBody Runs (8/17/2021)
We've taken down the old runs and replaced them with new ones:
We expect these runs to converge smoothly. If there are any problems, please do not hesitate to reach out.
Thank you all for your continued support,
17 Aug 2021, 20:25:14 UTC · Discuss
New Poll Regarding GPU Application of N-Body
We are currently looking at making a GPU version of N-Body. This code has been under development for quite some time, and the base code is finally working, though we would still need to implement some other features to run it alongside the CPU version. However, due to the complexity of our code and our need for double precision, the GPU version has a similar runtime to that of the CPU version, though there may be some speed-up on professional grade GPU cards. For reference, the GPU version of the Separation code is roughly 50-60 times faster than its CPU counterpart depending on the machine. Keeping that in mind, do you guys still want a GPU version of N-Body? I have put up a basic straw poll on https://www.strawpoll.me/45510486. If you wish to elaborate on your choice, please feel free to comment below.
Thank you all for your input, time, and consideration,
21 Jul 2021, 17:46:03 UTC · Discuss
Separation Validator Updates/Brief Server Outage(s)
I will be updating the separation validator starting at 3PM ET. The server will go down for a short time and then come back up. In the case that the new validator causes problems, the server will go back down again to revert to the old validator. I will be monitoring the situation and would appreciate input on any workunits that fail validation after the new validator goes live.
The server may go down/back up a few times during this process. Thanks for your patience. I'll keep you all posted on the status of things as they happen.
15 Jul 2021, 18:41:01 UTC · Discuss
New NBody Runs!
The last set of N-body runs has converged beautifully. Thus, we have replaced the old runs with a set of new ones:
Since the last set ran without problems, we expect this one to run smoothly, too. Thank you all for your continued support.
10 Jul 2021, 20:44:17 UTC · Discuss
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