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An Updated Characterization of Luminous Lyα Emitters at the End of Reionization

  • Authors: Yuanhang Ning, Zheng Cai, Linhua Jiang, Qiong Li, Si-Yue Yu, Xiaodi Yu, Zhen-Ya Zheng

Yuanhang Ning et al 2026 The Astrophysical Journal Letters 1009 .

  • Provider: AAS Journals

Caption: Figure 5.

SFR vs. M* diagram. The blue dashed line show the best-fit star-forming main sequence (SFMS) at 6 < z ≤ 7 obtained by L. Clarke et al. (2024). The magenta dashed lines represent the best-fit power-law relations from P. Rinaldi et al. (2022). The crosses indicate the z > 5 galaxies from M. Curti et al. (2024). The following open markers also represent the results from the literature. The square is LCEz4-M1, a LyC emitter (LCE) candidate at z = 4.444 reported by S. Zhu et al. (2026). The thin diamond is RXCJ2248, an N emitter at z = 8.05 from M. W. Topping et al. (2024). The thick diamonds are JADES-GS-z8-0-LA and JADES-GS-z8-1-LA, respectively, two z ∼ 8.5 LAEs with ﹩{f}_{{\rm{esc}}}^{{\rm{Ly}}\alpha }﹩ ∼ 10% from J. Witstok et al. (2025). The upward triangle is GN-z8-LAE, an LAE at z ≈ 8.3 from R. Navarro-Carrera et al. (2025). The downward triangle is a very blue starburst galaxy with ﹩{f}_{{\rm{esc}}}^{{\rm{LyC}}}﹩ ∼ 1 at z ∼ 10 reported by R. Marques-Chaves et al. (2026).

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