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No Luminous Little Red Dots: A Sharp Cutoff in Their Luminosity Function

  • Authors: Yilun Ma, 逸伦 马, Jenny E. Greene, Marta Volonteri, Andy D. Goulding, David J. Setton, Marianna Annunziatella, Eiichi Egami, Xiaohui Fan, Vasily Kokorev, Ivo Labbe, Xiaojing Lin, Danilo Marchesini, Jorryt Matthee, Themiya Nanayakkara, Luke Robbins, Anna Sajina, Marcin Sawicki

Yilun Ma et al 2026 The Astrophysical Journal Letters 1008 .

  • Provider: AAS Journals

Caption: Figure B1.

The observed and model photometry of ECOSMOS-LumLRD-z5 (circles and squares, respectively) is shown on top of the best-fit EAZY model (light blue curve with shades). The subcomponents of the best-fit model are shown with smaller line widths. Among all subcomponents, UNCOVER-45924, a JWST-selected LRD, is the most dominant component of all and is shown with thicker line width.

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