http://202.127.29.3/~shen/wiki/index.php?action=history&feed=atom&title=VIKINGVIKING - 版本历史2026-05-13T07:39:51Z本wiki上该页面的版本历史MediaWiki 1.38.1http://202.127.29.3/~shen/wiki/index.php?title=VIKING&diff=2412&oldid=prev2016年9月6日 (二) 12:23 Shen2016-09-06T12:23:29Z<p></p>
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<td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">2016年9月6日 (二) 12:23的版本</td>
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<td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* VIKING is the [[VISTA]] Kilo-degree Infrared Galaxy survey.</div></td>
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<td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>*overing the 1500 deg2 of the VST-KIDS survey in the 5 broadband filters Z,Y,J,H,Ks. Combined with [[KIDS]]</div></td>
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<td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>VIKING is a survey with [[VISTA]] covering the 1500 deg2 of the VST-KIDS survey in the 5 broadband filters Z,Y,J,H,Ks. Combined with [[KIDS]], this will yield a 9-band optical-IR survey with depth approximately 2 mag deeper than Sloan and 1.4 mag deeper than [[UKIDSS-LAS]]. The survey has numerous motivations including the highest redshift quasars, brown dwarfs, improved photometric redshifts for weak lensing and baryon oscillations, z > 1 clusters, stellar masses for the KIDS lensing objects, and studying galaxy evolution and clustering over the interval 0 < z < 1.2. In area and depth, the KIDS+VIKING survey is a natural intermediate between the shallower SDSS, VSTATLAS and UKIDSS-LAS, and the deeper 30 deg2 surveys. Some part of it is observable year-round from Paranal, providing a rich source of targets for VLT follow up.</div></td>
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</table>Shenhttp://202.127.29.3/~shen/wiki/index.php?title=VIKING&diff=587&oldid=prev202.127.29.127：以“* VIKING is the VISTA Kilo-degree Infrared Galaxy survey. VIKING is a survey with VISTA covering the 1500 deg2 of the VST-KIDS survey in the 5 broadband fil...”为内容创建页面2013-06-07T07:55:43Z<p>以“* VIKING is the <a href="/~shen/wiki/index.php/VISTA" title="VISTA">VISTA</a> Kilo-degree Infrared Galaxy survey. VIKING is a survey with <a href="/~shen/wiki/index.php/VISTA" title="VISTA">VISTA</a> covering the 1500 deg2 of the VST-KIDS survey in the 5 broadband fil...”为内容创建页面</p>
<p><b>新页面</b></p><div>* VIKING is the [[VISTA]] Kilo-degree Infrared Galaxy survey.<br />
<br />
VIKING is a survey with [[VISTA]] covering the 1500 deg2 of the VST-KIDS survey in the 5 broadband filters Z,Y,J,H,Ks. Combined with [[KIDS]], this will yield a 9-band optical-IR survey with depth approximately 2 mag deeper than Sloan and 1.4 mag deeper than [[UKIDSS-LAS]]. The survey has numerous motivations including the highest redshift quasars, brown dwarfs, improved photometric redshifts for weak lensing and baryon oscillations, z > 1 clusters, stellar masses for the KIDS lensing objects, and studying galaxy evolution and clustering over the interval 0 < z < 1.2. In area and depth, the KIDS+VIKING survey is a natural intermediate between the shallower SDSS, VSTATLAS and UKIDSS-LAS, and the deeper 30 deg2 surveys. Some part of it is observable year-round from Paranal, providing a rich source of targets for VLT follow up.</div>202.127.29.127