Photometric redshifts of emission-line galaxies
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Broadband photometric redshifts are routinely obtained for galaxies to estimate their distances. While effective for many uses, the common resolution in z of 0.01-0.02 is too...
天文研究中通常通过宽带测光红移(Broadband photometric redshifts)获取星系数据以估算其距离。尽管该方法在诸多应用场景中表现优异,但红移z方向的常规分辨率仅为0.01~0.02,仍过于……



