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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 10.

AGN–host image decomposition for HST ( top) and NIRCam ( bottom). Each cutout is 1﹩\mathop{.}\limits^{{\unicode{x02033}}}﹩5 × 1﹩\mathop{.}\limits^{{\unicode{x02033}}}﹩5. The first row shows the original image (total), followed by the host and AGN model components in the second and third rows, respectively. The final row displays the residuals, with overlaid contours highlighting the residual structures. All cutouts are shown using the same scale as the original image in each band.

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