| The evolution of radio-loud active galactic nuclei as a function of black hole spin D Garofalo, DA Evans, RM Sambruna Monthly Notices of the Royal Astronomical Society 406 (2), 975-986, 2010 | 205 | 2010 |
| The spin dependence of the blandford–znajek effect D Garofalo The Astrophysical Journal 699 (1), 400, 2009 | 96 | 2009 |
| Trapping of magnetic flux by the plunge region of a black hole accretion disk CS Reynolds, D Garofalo, MC Begelman The Astrophysical Journal 651 (2), 1023, 2006 | 96 | 2006 |
| A magnetohydrodynamic model of the M87 jet. i. superluminal knot ejections from HST-1 as trails of quad relativistic MHD shocks M Nakamura, D Garofalo, DL Meier The Astrophysical Journal 721 (2), 1783, 2010 | 51 | 2010 |
| FR0 radio galaxies and their place in the radio morphology classification D Garofalo, CB Singh The Astrophysical Journal 871 (2), 259, 2019 | 37 | 2019 |
| Black hole spin in AGN and GBHCs CS Reynolds, LW Brenneman, D Garofalo Astrophysics and Space Science 300, 71-79, 2005 | 29 | 2005 |
| Retrograde versus prograde models of accreting black holes D Garofalo Advances in Astronomy 2013 (1), 213105, 2013 | 26 | 2013 |
| Ransomware: The landscape is shifting-a concise report R Richardson, MM North, D Garofalo International Management Review 17 (1), 5-86, 2021 | 20 | 2021 |
| A unified framework for X-shaped radio galaxies D Garofalo, R Joshi, X Yang, CB Singh, M North, M Hopkins The Astrophysical Journal 889 (2), 91, 2020 | 20 | 2020 |
| Signatures of black hole spin in galaxy evolution D Garofalo The Astrophysical Journal 699 (1), L52, 2009 | 17 | 2009 |
| Why radio quiet quasars are preferred over radio loud quasars regardless of environment and redshift D Garofalo, M North, L Belga, K Waddell The Astrophysical Journal 890 (2), 144, 2020 | 15 | 2020 |
| Possible evolution of supermassive black holes from FRI quasars MI Kim, DJ Christian, D Garofalo, J D'Avanzo Monthly Notices of the Royal Astronomical Society 460 (3), 3221-3231, 2016 | 15 | 2016 |
| The Sub-Eddington Boundary for the Quasar Mass–Luminosity Plane: A Theoretical Perspective D Garofalo, DJ Christian, AM Jones Universe 5 (6), 145, 2019 | 12 | 2019 |
| Reconciling AGN-star formation, the Soltan argument, and Meier’s paradox D Garofalo, MI Kim, DJ Christian, E Hollingworth, A Lowery, M Harmon The Astrophysical Journal 817 (2), 170, 2016 | 12 | 2016 |
| The distribution and lifetime of powerful radio galaxies as a function of environment and redshift D Garofalo, CB Singh, A Zack Scientific Reports 8 (1), 15097, 2018 | 11 | 2018 |
| Constraints on the radio-loud/radio-quiet dichotomy from the Fundamental Plane D Garofalo, MI Kim, DJ Christian Monthly Notices of the Royal Astronomical Society 442 (4), 3097-3104, 2014 | 11 | 2014 |
| Sporadically torqued accretion disks around black holes D Garofalo, CS Reynolds The Astrophysical Journal 624 (1), 94, 2005 | 10 | 2005 |
| The jet–disc connection: evidence for a reinterpretation in radio loud and radio quiet active galactic nuclei D Garofalo Monthly Notices of the Royal Astronomical Society 434 (4), 3196-3201, 2013 | 9 | 2013 |
| The black hole-star formation connection over cosmic time CB Singh, N Kulasiri, M North, D Garofalo Publications of the Astronomical Society of the Pacific 133 (1028), 104101, 2021 | 8 | 2021 |
| The Distribution of Radio Quiet Active Galactic Nuclei in the Star Formation Rate-stellar Mass Plane D Garofalo, G Mountrichas Publications of the Astronomical Society of the Pacific 134 (1036), 064102, 2022 | 7 | 2022 |
Chandra Bahadur SinghAssociate Research Professor, South-Western Institute for Astronomy Research, Yunnan University在 ynu.edu.cn 的电子邮件经过验证
