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Beyond the Monsters: A More Complete Census of Black Hole Activity at Cosmic Dawn

  • Authors: Madisyn Brooks, Jonathan R. Trump, Raymond C. Simons, Justin Cole, Anthony J. Taylor, Micaela B. Bagley, Steven L. Finkelstein, Kelcey Davis, Ricardo O. Amorín, Bren E. Backhaus, Nikko J. Cleri, Mauro Giavalisco, Norman A. Grogin, Michaela Hirschmann, Benne W. Holwerda, Marc Huertas-Company, Jeyhan S. Kartaltepe, Dale D. Kocevski, Anton M. Koekemoer, Ray A. Lucas, Fabio Pacucci, Xin Wang

Madisyn Brooks et al 2026 The Astrophysical Journal 1002 .

  • Provider: AAS Journals

Caption: Figure 2.

Median Hα emission lines for our 16 stacks. Stacks increase in continuum luminosity from left to right, and increase in redshift from top to bottom. The total best-fit model is shown in purple for each stack, and a well-detected (>3σ) BL fit component is shown by the dashed red line. The ΔBIC, FWHM, and LHα,broad are given for each stack. Stacks that pass our three criteria for a detected BL, described in Section 4, have their ΔBIC, FWHM, and LHα,broad shown in red and a white background. Stacks that do not pass the BL identification criteria have a light gray background.

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