SED fitting results of HETDEX pilot survey
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https://b2find.eudat.eu/dataset/6160982f-40f4-5112-9835-419f842b66c5
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We use broadband photometry extending from the rest-frame UV to the near-IR to fit the individual spectral energy distributions of 63 bright (L(Ly{alpha})>10^43^ erg/s)...
我们采用覆盖静止帧紫外(rest-frame UV)至近红外(near-IR)波段的宽带测光数据,对63颗莱曼α光度$L( ext{Ly}alpha)>10^{43}$ 尔格/秒的明亮天体的个体光谱能量分布(Spectral Energy Distribution,SED)进行拟合……



