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COSMOS2020: Investigating the AGN-obscured accretion phase at z ∼ 1 via [Ne V] selection
L. Barchiesi, C. Vignali, F. Pozzi, R. Gilli, M. Mignoli, C. Gruppioni, A. Lapi, S. Marchesi, F. Ricci and C. M. Urry Astronomy & Astrophysics 685 A141 (2024) https://doi.org/10.1051/0004-6361/202245288
AGN impact on the molecular gas in galactic centres as probed by CO lines
Federico Esposito, Livia Vallini, Francesca Pozzi, et al. Monthly Notices of the Royal Astronomical Society 512(1) 686 (2022) https://doi.org/10.1093/mnras/stac313
The PEP survey: evidence for intense star-forming activity in the majority of radio-selected AGN atz≳ 1
M. Magliocchetti, D. Lutz, P. Santini, et al. Monthly Notices of the Royal Astronomical Society 456(1) 431 (2016) https://doi.org/10.1093/mnras/stv2645
Tracing black hole accretion with SED decomposition and IR lines: from local galaxies to the high-zUniverse
C. Gruppioni, S. Berta, L. Spinoglio, et al. Monthly Notices of the Royal Astronomical Society 458(4) 4297 (2016) https://doi.org/10.1093/mnras/stw577
The XMM–Newton Bright Survey sample of absorbed quasars: X-ray and accretion properties
L. Ballo, P. Severgnini, R. Della Ceca, et al. Monthly Notices of the Royal Astronomical Society 444(3) 2580 (2014) https://doi.org/10.1093/mnras/stu1628
ALMA reveals a warm and compact starburst around a heavily obscured supermassive black hole atz= 4.75
Three active galactic nuclei close to the effective Eddington limit for dusty gas
R. V. Vasudevan, A. C. Fabian, R. F. Mushotzky, et al. Monthly Notices of the Royal Astronomical Society 431(4) 3127 (2013) https://doi.org/10.1093/mnras/stt389
The AGN content in luminous infrared galaxies at z∼ 2 from a global SED analysis including Herschel data
Infrared spectra of the protonated neurotransmitter histamine: competition between imidazolium and ammonium isomers in the gas phase
Anita Lagutschenkov, Judith Langer, Giel Berden, Jos Oomens and Otto Dopfer Physical Chemistry Chemical Physics 13(34) 15644 (2011) https://doi.org/10.1039/c1cp21681c
Defining the intrinsic AGN infrared spectral energy distribution and measuring its contribution to the infrared output of composite galaxies★