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Porquet, D, Done, C, Reeves, JN, Grosso, N, Marinucci, A, Matt, G, Lobban, A ORCID: https://orcid.org/0000-0002-6433-1357, Nardini, E, Braito, V, Marin, F, Kubota, A, Ricci, C, Koss, M, Stern, D, Ballantyne, D and Farrah, D (2019) A deep X-ray view of the bare AGN Ark 120 - V. Spin determination from disc-Comptonisation efficiency method. Astronomy and Astrophysics, 623. A11 - A11.

Marinucci, A, Porquet, D, Tamborra, F, Bianchi, S, Braito, V, Lobban, A ORCID: https://orcid.org/0000-0002-6433-1357, Marin, F, Matt, G, Middei, R, Nardini, E, Reeves, J and Tortosa, A (2019) A deep X-ray view of the bare AGN Ark 120 - VI. Geometry of the hot corona from spectroscopic and polarization signatures. Astronomy and Astrophysics, 623. A12 -A12.

Porquet, D, Reeves, JN, Matt, G, Marinucci, A, Nardini, E, Braito, V, Lobban, AP ORCID: https://orcid.org/0000-0002-6433-1357, Ballantyne, DR, Boggs, SE, Christensen, FE, Dauser, T, Farrah, D, Garcia, J, Hailey, CJ, Harrison, F, Stern, D, Tortosa, A, Ursini, F and Zhang, WW (2018) A deep X-ray view of the bare AGN Ark120. IV. XMM-Newton and NuSTAR spectra dominated by two temperature (warm, hot) Comptonization processes. Astronomy & Astrophysics, 609. A42 -?.

Lobban, AP ORCID: https://orcid.org/0000-0002-6433-1357, Porquet, D, Reeves, JN, Markowitz, A, Nardini, E and Grosso, N (2017) A deep X-ray view of the bare AGN Ark 120. III. X-ray timing analysis and multiwavelength variability. Monthly Notices of the Royal Astronomical Society, 474 (3). pp. 3237-3258.

Reeves, JN, Braito, V, Behar, E, Fischer, T, Kraemer, S, Lobban, AP ORCID: https://orcid.org/0000-0002-6433-1357, Nardini, E, Porquet, D and Turner, J (2017) High Resolution X-ray Spectroscopy of the Seyfert 1, Mrk 1040. Revealing the Failed Nuclear Wind with Chandra. The Astrophysical Journal.

Reeves, JN, Porquet, D, Braito, V, Nardini, E, Lobban, AP ORCID: https://orcid.org/0000-0002-6433-1357 and Turner, J (2016) A deep X-ray view of the bare AGN Ark 120. I. Revealing the Soft X-ray Line Emission. Astrophysical Journal, 828 (2).