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Probing star formation rates and histories in AGN and non-AGN galaxies across diverse cosmic environments and X-ray luminosity ranges
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Comparative analysis of the SFR of AGN and non-AGN galaxies, as a function of stellar mass, AGN power, cosmic time, and obscuration
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Genuine Retrieval of the AGN Host Stellar Population (GRAHSP)
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A CIGALE module tailored (not only) for low-luminosity active galactic nuclei
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The co-evolution of supermassive black holes and galaxies in luminous AGN over a wide range of redshift
CEERS Key Paper. II. A First Look at the Resolved Host Properties of AGN at 3 < z < 5 with JWST
Dale D. Kocevski, Guillermo Barro, Elizabeth J. McGrath, Steven L. Finkelstein, Micaela B. Bagley, Henry C. Ferguson, Shardha Jogee, Guang Yang, Mark Dickinson, Nimish P. Hathi, Bren E. Backhaus, Eric F. Bell, Laura Bisigello, Véronique Buat, Denis Burgarella, Caitlin M. Casey, Nikko J. Cleri, M. C. Cooper, Luca Costantin, Darren Croton, Emanuele Daddi, Adriano Fontana, Seiji Fujimoto, Jonathan P. Gardner, Eric Gawiser, et al. The Astrophysical Journal Letters 946(1) L14 (2023) https://doi.org/10.3847/2041-8213/acad00
The relation of cosmic environment and morphology with the star formation and stellar populations of AGN and non-AGN galaxies
G. Mountrichas, G. Yang, V. Buat, B. Darvish, M. Boquien, Q. Ni, D. Burgarella and L. Ciesla Astronomy & Astrophysics 675 A137 (2023) https://doi.org/10.1051/0004-6361/202346706
Probing supermassive black hole growth and its dependence on stellar mass and star formation rate in low-redshift galaxies
O Torbaniuk, M Paolillo, R D’Abrusco, C Vignali, A Georgakakis, F J Carrera and F Civano Monthly Notices of the Royal Astronomical Society 527(4) 12091 (2023) https://doi.org/10.1093/mnras/stad3965
X-ray luminosity-star formation rate scaling relation: Constraints from the eROSITA Final Equatorial Depth Survey (eFEDS)
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Comparing the host galaxy ages of X-ray selected AGN in COSMOS
Testing the evolutionary pathways of galaxies and their supermassive black holes and the impact of feedback from active galactic nuclei via large multiwavelength data sets