First author publications: 14 – Co-author publications: 9 – H-index = 7 – G-index = 10 – Updated publication list: E. Kammoun ADS library 23. P. Draghis, …, E. S. Kammoun, et al., The Spin and Orientation of the Black Hole in XTE J1908+094, 2021, Accepted for publication in ApJ, preprint: ArXiv: 2107.02810. 22. J. M. Miller, …, E. S. Kammoun, et al., The Inner Accretion Flow in the Resurgent Seyfert-1.2 AGN Mrk 817, 2021, ApJL, 911, L12, DOI: 10.3847/2041-8213/abef6f. 21. E. S. Kammoun, I. E. Papadakis, M. Dovciak, Modeling the UV/optical continuum time-lags in AGN, 2021, Accepted for publication in MNRAS, DOI: 10.1093/mnras/stab725 20. B. Balakrishnan, …, E. S. Kammoun, et al. The novel obscured state of stellar-mass black hole GRS 1915+105, 2021, ApJ, 909, 41, DOI: 10.3847/1538-4357/abd6cb. 19. E. S. Kammoun, M. Dovciak, I. E. Papadakis, et al. Thermal reverberation in Active Galactic Nuclei, 2021, ApJ, 907, 20, DOI: 10.3847/1538-4357/abcb93. 18. J. M. Miller, …, E. S. Kammoun, et al., An Obscured, Seyfert 2-like State of the Stellar-mass Black Hole GRS 1915+105 Caused by Failed Disk Winds, 2020, ApJ, 904, 30, DOI: 10.3847/1538-4357/abbb31. 17. C. Panagiotou, I. E. Papadakis, E. S. Kammoun & M. Dovciak, Multiwavelength power-spectrum analysis of NGC 5548, 2020, MNRAS, 499 (2), 1998, DOI: 10.1093/mnras/staa2920. 16. E. S. Kammoun, J. M. Miller, M. Koss, et al., 2020, A hard look at local, optically-selected, obscured Seyfert galaxies, 2020, ApJ, 901, 161, DOI: 10.3847/1538-4357/abb29f. 15. G. Matzeu, …, E. S. Kammoun, et al., The first broadband X-ray view of the narrow line Seyfert 1 Ton S180, 2020, MNRAS, 497, 2352, DOI: 10.1093/mnras/staa2076. 14. P. Draghis, …, E. S. Kammoun, et al., A New Spin on an Old Black Hole: NuSTAR Spectroscopy of EXO 1846−031, 2020, ApJ, 900, 78, DOI: 10.3847/1538-4357/aba2ec. 13. E. S. Kammoun, E. Nardini, A. Zoghbi, et al. The nature of the broadband X-ray variability in the dwarf Seyfert galaxy NGC 4395, 2019, ApJ, 886, 145, DOI: 10.3847/1538-4357/ab5110. 12. J. M. Miller, E. S. Kammoun et al. A NICER Look at Strong X-ray Obscuration in the Seyfert-2 Galaxy NGC 4388, 2019, ApJ, 884, 106, DOI: 10.3847/1538-4357/ab3e05. 11. E. S. Kammoun, I. E. Papadakis & M. Dovciak, A Hard Look at Thermal Reverberation and Optical/UV lags in NGC 5548, 2019, ApJL, 879, L24, DOI: 10.3847/2041-8213/ab2a72. 10. E. S. Kammoun, J. M. Miller, A. Zoghbi, et al., A Hard look at NGC 5347: Revealing a Nearby Compton￾thick AGN, 2019, ApJ, 877, 102, DOI: 10.3847/1538-4357/ab1c5f. 9. E. S. Kammoun, V. Domcek, J. Svoboda et al., Steep X-ray reflection emissivity profiles in AGN as the result of radially structured disc ionization, 2019, MNRAS, 485 (1), 239, DOI: 10.1093/mnras/stz408. 8. E. S. Kammoun & I. E. Papadakis, The nature of X-ray spectral variability in SWIFT J2127.4+5654, 2018, MNRAS, 480 (3), 3412, DOI: 10.1093/mnras/sty2067. 7. E. S. Kammoun, F. Marin, M. Dovciak et al., X-ray spectral and polarimetric signatures of X-ray eclipses in AGN, 2018, MNRAS, 480 (3), 3243, DOI: 10.1093/mnras/sty2084. 6. F. Marin, M. Dovciak & E. S. Kammoun, Contribution of parsec-scale material onto the polarized X-ray spectrum of type-1 Seyfert galaxies, 2018, MNRAS, 478, 950, DOI: 10.1093/mnras/sty1062 . 5. E. S. Kammoun, E. Nardini & G. Risaliti, Testing the accuracy of reflection-based supermassive black hole spin measurements in AGN, 2018, A&A, 614. A44, DOI: 10.1051/0004-6361/201732377. 4. E. S. Kammoun, E. Nardini, G. Risaliti et al., Bulk Comptonization: new hints from the luminous blazar 4C+25.05, 2018, MNRASL, 473 (1), L89, DOI: 10.1093/mnrasl/slx164. 3. E. S. Kammoun & I. E. Papadakis, The nature of X-ray spectral variability in MCG–6-30-15, 2017, MNRAS, 472 (3), 3131, DOI: 10.1093/mnras/stx2181. 2. E. S. Kammoun, G. Risaliti, D. Stern et al., Coronal properties of the luminous radio-quiet quasar QSO B2202-209, 2017, MNRAS, 465 (2), 1665, DOI: 10.1093/mnras/stw2897 1. E. S. Kammoun, I. E. Papadakis, & B. M. Sabra, Variability of the soft X-ray excess in IRAS 13224−3809, 2015, A&A, 582, A40, DOI: 10.1051/0004-6361/201526811.