查看“JWST”的源代码

==NIRspec==
*NIRSpec is equipped with an integral field unit optimized for the spectroscopic study of complex extended objects. It will provide 900 spectra per exposure over a field of view of 3 x 3 arcminutes.（0.6-5mu）

==MIRI==
*用CAFE拟合，可以得到9.7mu的尘埃光深
*H2的转动线S(1)-S(7)，可以直接测量H2的含量
*[Ne iii]1.56mu/[Ne ii]12.81mu, which is an indicator of the hardness of the local radiation field
*“The SFR  can be estimated with the Pf α, [Ne ii], and [Ne iii] measurements. By assuming a Case B scenario， we translate our Pf α flux to Hα and apply Equation (2) in Murphy et al. (2011) to derive the SFR in our extracted regions.
* 可以用image-registration的方法来把图对齐，从而解天体测量。https://doi.org/10.3847/2041-8213/acaaae

==sciences==
* 高红移spiral星系的比例挺高的，至少20% @z~3 [https://arxiv.org/pdf/2312.12389.pdf]
==projects==
*[[JADES]]

==data==
*DAWN JWST Archive [https://dawn-cph.github.io/dja/about/summary/]