TheSkyNet POGS: Difference between revisions
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{{Infobox software | {{Infobox software | ||
| name = theSkyNet POGS | | name = theSkyNet POGS | ||
| logo = | | logo = POGS-Reverse.png | ||
| logo caption = | | logo caption = | ||
| screenshot = NGC 2703 PanS.jpg | | screenshot = NGC 2703 PanS.jpg | ||
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| operating system = Windows, Unix/Linux, macOS, Android<ref name="wiki-theskynet" /> | | operating system = Windows, Unix/Linux, macOS, Android<ref name="wiki-theskynet" /> | ||
| size = | | size = | ||
| stats as of = {{Start date and age| | | stats as of = {{Start date and age|2018|04|07}} | ||
| average performance = | | average performance = 94884.68 GigaFLOPS | ||
| active users = | | active users = 7711 | ||
| total users = | | total users = 65332 | ||
| active hosts = | | active hosts = 19904 | ||
| total hosts = | | total hosts = 361195 | ||
| rac = | | rac = | ||
| credit per day = | | credit per day = | ||
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{{Lowercase title}} | {{Lowercase title}} | ||
'''theSkyNet POGS''' ('''P'''an-STARRS '''O'''ptical '''G'''alaxy '''S'''urvey) was a [[wikipedia:volunteer computing|volunteer computing]] project that used [[wikipedia:BOINC|BOINC]] to measure the physical properties of tens of thousands of nearby galaxies. It was run by the [[wikipedia:International Centre for Radio Astronomy Research|International Centre for Radio Astronomy Research]] (ICRAR), a joint venture of [[wikipedia:Curtin University|Curtin University]] and the [[wikipedia:University of Western Australia|University of Western Australia]], as one of two research projects under the umbrella of '''theSkyNet''', ICRAR's public astronomy outreach initiative.<ref name="wiki-theskynet">{{Cite web |title=TheSkyNet |url=https://en.wikipedia.org/wiki/TheSkyNet |website=Wikipedia |access-date=2026-07-16}}</ref> POGS combined imaging from three space telescopes, [[wikipedia:GALEX|GALEX]], [[wikipedia:Pan-STARRS|Pan-STARRS1]] and [[wikipedia:Wide-field Infrared Survey Explorer|WISE]], to build a multi-wavelength, pixel-resolved atlas of galaxy properties such as stellar mass, star formation rate and dust content.<ref name="vinsen2013" /> theSkyNet POGS was the first Australian-based project to be made available to the public on BOINC.<ref name="icrar-t2">{{Cite web |title=theSkyNet: T2 is Born |url=https://www.icrar.org/theskynet-t2-born/ |publisher=ICRAR |date=2012-09-13 |access-date=2026-07-16}}</ref> | '''[https://web.archive.org/web/20130725025029/http://pogs.theskynet.org/pogs/ theSkyNet POGS]''' ('''P'''an-STARRS '''O'''ptical '''G'''alaxy '''S'''urvey) was a [[wikipedia:volunteer computing|volunteer computing]] project that used [[wikipedia:BOINC|BOINC]] to measure the physical properties of tens of thousands of nearby galaxies. It was run by the [[wikipedia:International Centre for Radio Astronomy Research|International Centre for Radio Astronomy Research]] (ICRAR), a joint venture of [[wikipedia:Curtin University|Curtin University]] and the [[wikipedia:University of Western Australia|University of Western Australia]], as one of two research projects under the umbrella of '''theSkyNet''', ICRAR's public astronomy outreach initiative.<ref name="wiki-theskynet">{{Cite web |title=TheSkyNet |url=https://en.wikipedia.org/wiki/TheSkyNet |website=Wikipedia |access-date=2026-07-16}}</ref> POGS combined imaging from three space telescopes, [[wikipedia:GALEX|GALEX]], [[wikipedia:Pan-STARRS|Pan-STARRS1]] and [[wikipedia:Wide-field Infrared Survey Explorer|WISE]], to build a multi-wavelength, pixel-resolved atlas of galaxy properties such as stellar mass, star formation rate and dust content.<ref name="vinsen2013" /> theSkyNet POGS was the first Australian-based project to be made available to the public on BOINC.<ref name="icrar-t2">{{Cite web |title=theSkyNet: T2 is Born |url=https://www.icrar.org/theskynet-t2-born/ |publisher=ICRAR |date=2012-09-13 |access-date=2026-07-16}}</ref> | ||
The project completed its data-processing goals in May 2018 and is no longer distributing work.<ref name="pogscomplete" /> | The project completed its data-processing goals in May 2018 and is no longer distributing work.<ref name="pogscomplete" /> | ||