An Introduction of A Data-driven Model for Analyzing Stellar Spectra
This thesis describes a method for concluding attributes of a star (including ages, temperatures, chemical element abundances) from its spectra. The method was developed by the 4MOST (4-metre Multi-Object Spectroscopic Telescope) consortium. How the model outputs stellar attributes by receiving spectra is too complicated to be included in one thesis, so only introductions of numerical methods whic
