https://boincsynergy.ca/wiki/api.php?action=feedcontributions&feedformat=atom&user=129.161.156.172 2026-05-31T18:06:02Z User contributions MediaWiki 1.43.8 https://boincsynergy.ca/wiki/index.php?title=MilkyWay@home&diff=804 2024-05-03T20:54:32Z

<p>129.161.156.172: Addign to why milkyway@home</p> <hr /> <div>&lt;div style=&quot;background-color: #D4E2FC; border-top: 1px solid #5F92F2; font-size: bigger; padding-left: 15px; margin: 12px -5px -5px -5px;&quot;&gt;'''BOINC project page template'''&lt;/div&gt;<br /> <br /> [[File:{{#setmainimage:Mw.png}}|alt=MilkyWay@home image|center|frameless]]<br /> <br /> [https://milkyway.cs.rpi.edu/milkyway/ '''''MilkyWay@home'''''] is a '''''[[wikipedia:Volunteer computing|volunteer distributed computing]]''''' project based at [https://www.rpi.edu/ '''''Rensselaer Polytechnics Institute'''''] that needs your help to optimize N-body simulations of dwarf galaxies around the Milky Way.<br /> <br /> == Why MilkyWay@home? ==<br /> The N-body project on MilkyWay@home simulates dwarf galaxies colliding with (or being disrupted by) the Milky Way. The result from this project will give insight on how dwarf galaxies interact with the Milky Way given certain parameters and how those results look when compared to the data observed today. <br /> <br /> == Goal ==<br /> The goal of the N-body project is to match simulated dwarf galaxies to real dwarf galaxy data, and thereby constrain the properties of the Milky Way galaxy's gravitational potential (as well as the properties of the dwarf galaxies).<br /> <br /> == Methods ==<br /> * always including &quot;why BOINC&quot;?<br /> [[File:Milkyway.gif|alt=Milky Way image|none|thumb|A dwarf galaxy being disrupted by the Milky Way's gravity (the Milky Way is not shown, and would be at the center of the picture)]]<br /> <br /> * impactful final statement<br /> <br /> == Project team / Sponsors ==<br /> <br /> *<br /> <br /> == Project results ==<br /> https://milkyway.cs.rpi.edu/milkyway/information.php<br /> <br /> == Scientific publications ==<br /> https://boinc.berkeley.edu/pubs.php#Milkyway@home</div>

129.161.156.172 https://boincsynergy.ca/wiki/index.php?title=MilkyWay@home&diff=803 2024-05-03T20:48:45Z

<p>129.161.156.172: adding hyperlink for RPI</p> <hr /> <div>&lt;div style=&quot;background-color: #D4E2FC; border-top: 1px solid #5F92F2; font-size: bigger; padding-left: 15px; margin: 12px -5px -5px -5px;&quot;&gt;'''BOINC project page template'''&lt;/div&gt;<br /> <br /> [[File:{{#setmainimage:Mw.png}}|alt=MilkyWay@home image|center|frameless]]<br /> <br /> [https://milkyway.cs.rpi.edu/milkyway/ '''''MilkyWay@home'''''] is a '''''[[wikipedia:Volunteer computing|volunteer distributed computing]]''''' project based at [https://www.rpi.edu/ '''''Rensselaer Polytechnics Institute'''''] that needs your help to optimize N-body simulations of dwarf galaxies around the Milky Way.<br /> <br /> == Why MilkyWay@home? ==<br /> The N-body project on MilkyWay@home simulates dwarf galaxies colliding with (or being disrupted by) the Milky Way. <br /> <br /> == Goal ==<br /> The goal of the N-body project is to match simulated dwarf galaxies to real dwarf galaxy data, and thereby constrain the properties of the Milky Way galaxy's gravitational potential (as well as the properties of the dwarf galaxies).<br /> <br /> == Methods ==<br /> * always including &quot;why BOINC&quot;?<br /> [[File:Milkyway.gif|alt=Milky Way image|none|thumb|A dwarf galaxy being disrupted by the Milky Way's gravity (the Milky Way is not shown, and would be at the center of the picture)]]<br /> <br /> * impactful final statement<br /> <br /> == Project team / Sponsors ==<br /> <br /> *<br /> <br /> == Project results ==<br /> https://milkyway.cs.rpi.edu/milkyway/information.php<br /> <br /> == Scientific publications ==<br /> https://boinc.berkeley.edu/pubs.php#Milkyway@home</div>

129.161.156.172 https://boincsynergy.ca/wiki/index.php?title=MilkyWay@home&diff=802 2024-05-03T20:47:16Z

<p>129.161.156.172: Beginning to add info to page</p> <hr /> <div>&lt;div style=&quot;background-color: #D4E2FC; border-top: 1px solid #5F92F2; font-size: bigger; padding-left: 15px; margin: 12px -5px -5px -5px;&quot;&gt;'''BOINC project page template'''&lt;/div&gt;<br /> <br /> [[File:{{#setmainimage:Mw.png}}|alt=MilkyWay@home image|center|frameless]]<br /> <br /> [https://milkyway.cs.rpi.edu/milkyway/ '''''MilkyWay@home'''''] is a '''''[[wikipedia:Volunteer computing|volunteer distributed computing]]''''' project based at Rensselaer Polytechnics Institute that needs your help to optimize N-body simulations of dwarf galaxies around the Milky Way.<br /> <br /> == Why MilkyWay@home? ==<br /> The N-body project on MilkyWay@home simulates dwarf galaxies colliding with (or being disrupted by) the Milky Way. <br /> <br /> == Goal ==<br /> The goal of the N-body project is to match simulated dwarf galaxies to real dwarf galaxy data, and thereby constrain the properties of the Milky Way galaxy's gravitational potential (as well as the properties of the dwarf galaxies).<br /> <br /> == Methods ==<br /> * always including &quot;why BOINC&quot;?<br /> [[File:Milkyway.gif|alt=Milky Way image|none|thumb|A dwarf galaxy being disrupted by the Milky Way's gravity (the Milky Way is not shown, and would be at the center of the picture)]]<br /> <br /> * impactful final statement<br /> <br /> == Project team / Sponsors ==<br /> <br /> *<br /> <br /> == Project results ==<br /> https://milkyway.cs.rpi.edu/milkyway/information.php<br /> <br /> == Scientific publications ==<br /> https://boinc.berkeley.edu/pubs.php#Milkyway@home</div>

129.161.156.172