“SAMI”的版本间差异
跳到导航
跳到搜索
无编辑摘要 |
无编辑摘要 |
||
| 第1行： | 第1行： | ||
'''Sydney-AAO Multi-object Integral field spectrograph (SAMI)''' |
'''Sydney-AAO Multi-object Integral field spectrograph (SAMI)''' |
||
* 13 integral field units (IFUs),each with a field of view of 15arcsec |
* 13 integral field units (IFUs),each with a field of view of 15arcsec and 61 packed fibers |
||
* each IFU consists of a bundle of 61 optical fibers a high filling factor ~75%) |
* each IFU consists of a bundle of 61 optical fibers a high filling factor ~75%) |
||
* installed on the 3.9-m Anglo-Australian Telescope (AAT) |
* installed on the 3.9-m Anglo-Australian Telescope (AAT),1 deg FOV |
||
* 370–570 nm with R=1730 in the blue arm, and 625–735 nm with R = 4500 in the red arm. |
* 370–570 nm with R=1730 in the blue arm, and 625–735 nm with R = 4500 in the red arm. |
||
---- |
---- |
||
2016年3月9日 (三) 11:16的版本
Sydney-AAO Multi-object Integral field spectrograph (SAMI)
- 13 integral field units (IFUs),each with a field of view of 15arcsec and 61 packed fibers
- each IFU consists of a bundle of 61 optical fibers a high filling factor ~75%)
- installed on the 3.9-m Anglo-Australian Telescope (AAT),1 deg FOV
- 370–570 nm with R=1730 in the blue arm, and 625–735 nm with R = 4500 in the red arm.
SAMI Galaxy survey
- aim: IFS data for 3400 galaxies
- Sample:
- a field and group sample from GAMA G09, G12 and G15 fields
- a cluster sample from a set of eight galaxy clusters.
- EDR, 107 galaxies [1]