“星系巡天”的版本间差异
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无编辑摘要 |
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:MASSIVE is a volume-limited sample of the 116 most massive early-type galaxies within 108 Mpc(Mk<-25.3). |
:MASSIVE is a volume-limited sample of the 116 most massive early-type galaxies within 108 Mpc(Mk<-25.3). |
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:IFS (107"x107") taken with the Mitchell Spectrograph on the 2.7m Harlan J. Smith telescope at the McDonald Observatory (Green et al. 2013) |
:IFS (107"x107") taken with the Mitchell Spectrograph on the 2.7m Harlan J. Smith telescope at the McDonald Observatory (Green et al. 2013) |
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*KMOS |
*KMOS |
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:The K-band Multi Object Spectrograph (KMOS). IFS in the near-infrared bands for 24 targets simultaneously. |
:The K-band Multi Object Spectrograph (KMOS). IFS in the near-infrared bands for 24 targets simultaneously. |
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==Keck上的终端== |
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*MOSFIRE |
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:Multi-Object Spectrometer for Infra-Red Exploration |
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===100%filling IFUs=== |
===100%filling IFUs=== |
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2016年6月15日 (三) 03:04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.
Keck上的终端
- MOSFIRE
- Multi-Object Spectrometer for Infra-Red Exploration
100%filling IFUs
- SAURON:33"x4"
- WiFeS:38"x25"