“星系巡天”的版本间差异
跳到导航
跳到搜索
（→红移巡天） |
（→IFS） |
||
| 第62行： | 第62行： | ||
[[LEGA-C]] |
[[LEGA-C]] |
||
== |
==IFS== |
||
*[[CALIFA]] |
*[[CALIFA]] |
||
*[[CHILI]] |
*[[CHILI]] |
||
*[[MaNGA]]: 同时17个源 |
*[[MaNGA]]: 同时17个源 |
||
*[[SAMI]]: 同时观测12个源 |
*[[SAMI]]: 同时观测12个源 |
||
*[[MASSIVE]] galaxy survey [Ma et al. 2014] |
|||
:MASSIVE is a volume-limited sample of the 116 most massive early-type galaxies within 108 Mpc(Mk<-25.3). |
|||
:IFS (107"x107") taken with the Mitchell Spectrograph on the 2.7m Harlan J. Smith telescope at the McDonald Observatory (Green et al. 2013) |
|||
===VLT上的两个IFS终端=== |
===VLT上的两个IFS终端=== |
||
2016年4月8日 (五) 05:55的版本
综合
测光巡天
AEGIS:2007
COSMOS:2008
VIKINGongoing
红移巡天
IFS
- MASSIVE is a volume-limited sample of the 116 most massive early-type galaxies within 108 Mpc(Mk<-25.3).
- IFS (107"x107") taken with the Mitchell Spectrograph on the 2.7m Harlan J. Smith telescope at the McDonald Observatory (Green et al. 2013)
VLT上的两个IFS终端
- MUSE
- a giant IFS on VLT wth 1 arcmin FoV, 0.2" spaxel
- KMOS
- The K-band Multi Object Spectrograph (KMOS). IFS in the near-infrared bands for 24 targets simultaneously.
100%filling IFUs
- SAURON:33"x4"
- WiFeS:38"x25"