查看“WISE”的源代码

*40cm 口径
*WISE最终有一个all sky survey在4个波段。
:3.4mu(W1) 4.6mu(W2) 12mu(W3) 22mu(W4)
:在W1的角分辨率是6" (好像和GALEX比较相当）
:现在WISE的preliminary release source catalog (PSRC)覆盖57%的天区
*arXiv 1111.5450
:W1-W2红，说明尘埃里面有热（1000k）的组份，和SFR相关，SFR很大（UV辐射强），加热尘埃。
*arXiv 1411.5020
:W3-W2 trace f(H2),比如NUV-r还好
*对于尘埃温度比较低的红外辐射来说，W4上可能探测不到，而Herschel 250mu可以

==WISE color-color plot==
*W1-W2  VS W2-W4   (Tsai 2011)

==基于WISE的增值数据==
*Chang et al. SDSS+WISE stellar mass and SFR [http://adsabs.harvard.edu/abs/2015ApJS..219....8C]
*固定位置的测光 Dustin Lang et al.[http://adsabs.harvard.edu/abs/2016AJ....151...36L]

==WISE数据的相关研究==
* We find a highly significant correlation between the WISE 12 micron to 4.6 micron flux ratios and molecular gas fractions in both PSBs and normal galaxies. [https://arxiv.org/abs/1705.00668]