“SAMI”的版本间差异

2017年3月6日 (一) 05:29的最新版本

Sydney-AAO Multi-object Integral field spectrograph (SAMI)

12 galaxies and 1 secondary star

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

a field and group sample from GAMA G09, G12 and G15 fields

a cluster sample from a set of eight galaxy clusters.

数据预期在2018年释放

r<19.5

光谱处理

which utilizes pPXF for stellar template fitting and the MPFIT library (MILES templates) for estimating emission-line properties.

@@ 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
+:12 galaxies and 1 secondary star
 * 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.
 ----
-SAMI Galaxy survey
+'''SAMI Galaxy survey'''
-* IFS data for �3400 galaxies (goal)
+* 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.
+:: 数据预期在2018年释放
+:: r<19.5
-* Till 2014, Sep., 1000 has been observed
 * EDR, 107 galaxies [http://sami-survey.org/edr]
+----
+'''光谱处理'''
+*SAMI的光谱发射线拟合程序LZIFU,Ho et al. (2014)
+:which utilizes pPXF for stellar template  fitting and the MPFIT library (MILES templates) for estimating emission-line properties.