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(LRDs)2: The Low-ReDshift Little Red Dots Survey. II. DESI DR1 Sample

  • Authors: Xiaojing Lin, Xiaohui Fan, Zheng Cai, Yichen Liu, Fengwu Sun, Fuyan Bian, Mingyu Li, Junjie Mao, Jenny E. Greene, Hanpu Liu, Jiaxuan Li, 嘉轩 李, Weizhe Liu, 伟哲 刘, Yilun Ma, 逸伦 马, Zechang Sun, Zijian Zhang

Xiaojing Lin et al 2026 The Astrophysical Journal 1012 .

  • Provider: AAS Journals

Caption: Figure 2.

Example DESI DR1 LRDs presented in this work. The top panel shows the overall SEDs, with the smoothed DESI spectra plotted as blue lines and the photometry as blue squares. The gray lines indicate the spectral uncertainties. The orange dashed lines mark the Balmer-limit wavelengths, and the blue dashed lines indicate the inflection-point wavelengths. The bottom panel shows the Hβ [O III]λλ 4960, 5008 and Hα line profiles, with the red curves denoting the best-fit total models and the dashed lines representing the best-fit individual components.

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