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Beyond the Dot: An LRD-like Nucleus at the Heart of an IR-bright Galaxy and its Implications for High-redshift LRDs

  • Authors: Pierluigi Rinaldi, George H. Rieke, Zihao Wu, Carys J. E. Gilbert, Fabio Pacucci, Luigi Barchiesi, Stacey Alberts, Stefano Carniani, Andrew J. Bunker, Rachana Bhatawdekar, Francesco D'Eugenio, Zhiyuan Ji, Benjamin D. Johnson, Kevin Hainline, Vasily Kokorev, Nimisha Kumari, Edoardo Iani, Jianwei Lyu, Roberto Maiolino, Eleonora Parlanti, Brant E. Robertson, Yang Sun, Cristian Vignali, Christina C. Williams, Christopher N. A. Willmer, Yongda Zhu

Pierluigi Rinaldi et al 2026 The Astrophysical Journal 1006 .

  • Provider: AAS Journals

Caption: Figure 8.

Radial profiles of the stacked rest-frame UV (1500–2000 Å) images of photometrically selected LRDs from P. Rinaldi et al. (2025a), shown in redshift bins. For comparison, the nominal PSFs are overplotted: F115W for z ≈ 4–5.8 and F150W for z ≈ 5.8–8. A slight increase in radial extent is observed when moving from the highest to the lowest redshift bin.

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