“S4G”的版本间差异
跳到导航
跳到搜索
（以“*Spitzer Survey of Stellar Structure in Galaxies : a deep 3.6 and 4.5 $\mu$m imaging survey of 2352 nearby ($< 40$ Mpc) galaxies. :[http://arxiv.org/abs/1503.06...”为内容创建页面） |
无编辑摘要 |
||
| （未显示同一用户的1个中间版本） | |||
| 第1行： | 第1行： | ||
*[[Spitzer]] Survey of Stellar Structure in Galaxies |
*[[Spitzer]] Survey of Stellar Structure in Galaxies [http://arxiv.org/abs/1503.06550] |
||
: a deep 3.6 and 4.5 $\mu$m imaging survey of 2352 nearby ($< 40$ Mpc) galaxies. |
: a deep 3.6 and 4.5 $\mu$m imaging survey of 2352 nearby ($< 40$ Mpc) galaxies. |
||
:the S$^4$G data analysis pipeline 4, which is dedicated to 2-dimensional structural surface brightness decompositions of 3.6 $\mu$m images, using GALFIT3.0 \citep{peng2010}. |
|||
:[http://arxiv.org/abs/1503.06550] |
|||
2015年3月24日 (二) 04:46的最新版本
- a deep 3.6 and 4.5 $\mu$m imaging survey of 2352 nearby ($< 40$ Mpc) galaxies.
- the S$^4$G data analysis pipeline 4, which is dedicated to 2-dimensional structural surface brightness decompositions of 3.6 $\mu$m images, using GALFIT3.0 \citep{peng2010}.