“VIKING”的版本间差异

2016年9月6日 (二) 12:23的最新版本

overing the 1500 deg2 of the VST-KIDS survey in the 5 broadband filters Z,Y,J,H,Ks. Combined with KIDS
9-band optical-IR survey with depth approximately 2 mag deeper than Sloan and 1.4 mag deeper than UKIDSS-LAS.

VIKING 的z波段大概比SDSS的r波段深一等。

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.

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 * VIKING is the [[VISTA]] Kilo-degree Infrared Galaxy survey.
+*overing the 1500 deg2 of the VST-KIDS survey in the 5 broadband filters Z,Y,J,H,Ks. Combined with [[KIDS]]
-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.
+*9-band optical-IR survey with depth approximately 2 mag deeper than Sloan and 1.4 mag deeper than [[UKIDSS-LAS]].
+:VIKING 的z波段大概比SDSS的r波段深一等。
+*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.