On the importance of using appropriate spectral models to derive physical properties of galaxies at

来源 :2015年东亚青年天文学家会议 | 被引量 : 0次 | 上传用户:wusuowei2100
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Interpreting ultraviolet-to-infrared observations of distant galaxies in terms of constraints on physical parameters-such as stellar mass,star formation rate (SFR) and attenuation by dust-requires spectral synthesis modelling.
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