Theoretical modeling of starburst galaxies LJ Kewley, MA Dopita, RS Sutherland, CA Heisler, J Trevena The Astrophysical Journal 556 (1), 121, 2001 | 2947 | 2001 |
Cooling functions for low-density astrophysical plasmas RS Sutherland, MA Dopita Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 88, no. 1, p …, 1993 | 2940 | 1993 |
Spectral signatures of fast shocks. II. Optical diagnostic diagrams MA Dopita, RS Sutherland Astrophysical Journal v. 455, p. 468 455, 468, 1995 | 764 | 1995 |
Spectral signatures of fast shocks. I. Low-density model grid MA Dopita, RS Sutherland Astrophysical Journal Supplement v. 102, p. 161 102, 161, 1996 | 679 | 1996 |
Theoretical evolution of optical strong lines across cosmic time LJ Kewley, MA Dopita, C Leitherer, R Davé, T Yuan, M Allen, B Groves, ... The Astrophysical Journal 774 (2), 100, 2013 | 518 | 2013 |
Understanding galaxy evolution through emission lines LJ Kewley, DC Nicholls, RS Sutherland Annual Review of Astronomy and Astrophysics 57 (1), 511-570, 2019 | 440 | 2019 |
Astrophysics of the diffuse universe MA Dopita, RS Sutherland Springer Science & Business Media, 2013 | 400 | 2013 |
Dusty, radiation pressure-dominated photoionization. I. model description, structure, and grids BA Groves, MA Dopita, RS Sutherland The Astrophysical Journal Supplement Series 153 (1), 9, 2004 | 353 | 2004 |
A theoretical recalibration of the extragalactic H II region sequence MA Dopita, LJ Kewley, CA Heisler, RS Sutherland The Astrophysical Journal 542 (1), 224, 2000 | 353 | 2000 |
New strong-line abundance diagnostics for H ii regions: effects of κ-distributed electron energies and new atomic data MA Dopita, RS Sutherland, DC Nicholls, LJ Kewley, FPA Vogt The Astrophysical Journal Supplement Series 208 (1), 10, 2013 | 330 | 2013 |
Modeling the pan-spectral energy distribution of starburst galaxies. IV. The controlling parameters of the starburst SED B Groves, MA Dopita, RS Sutherland, LJ Kewley, J Fischera, C Leitherer, ... The Astrophysical Journal Supplement Series 176 (2), 438, 2008 | 301 | 2008 |
Chemical abundances in high-redshift galaxies: a powerful new emission line diagnostic MA Dopita, LJ Kewley, RS Sutherland, DC Nicholls Astrophysics and Space Science 361, 1-7, 2016 | 289 | 2016 |
Externally illuminated young stellar environments in the Orion Nebula: Hubble space telescope planetary camera and ultraviolet observations J Bally, RS Sutherland, D Devine, D Johnstone The Astronomical Journal 116 (1), 293, 1998 | 268 | 1998 |
Dusty, radiation pressure-dominated photoionization. II. Multiwavelength emission line diagnostics for narrow-line regions BA Groves, MA Dopita, RS Sutherland The Astrophysical Journal Supplement Series 153 (1), 75, 2004 | 266 | 2004 |
Are the narrow-line regions in active galaxies dusty and radiation pressure dominated? MA Dopita, BA Groves, RS Sutherland, L Binette, G Cecil The Astrophysical Journal 572 (2), 753, 2002 | 248 | 2002 |
Modeling the pan-spectral energy distribution of starburst galaxies. III. Emission line diagnostics of ensembles of evolving H II regions MA Dopita, J Fischera, RS Sutherland, LJ Kewley, C Leitherer, RJ Tuffs, ... The Astrophysical Journal Supplement Series 167 (2), 177, 2006 | 237 | 2006 |
A database for galaxy evolution modeling C Leitherer, D Alloin, UFV Alvensleben, JS Gallagher, JP Huchra, ... Publications of the Astronomical Society of the Pacific 108 (729), 996, 1996 | 237 | 1996 |
CHIANTI—an atomic database for emission lines. XV. Version 9, improvements for the X-ray satellite lines KP Dere, G Del Zanna, PR Young, E Landi, RS Sutherland The Astrophysical Journal Supplement Series 241 (2), 22, 2019 | 231 | 2019 |
Resolving the electron temperature discrepancies in H II regions and planetary nebulae: κ-distributed electrons DC Nicholls, MA Dopita, RS Sutherland The Astrophysical Journal 752 (2), 148, 2012 | 226 | 2012 |
Jet-induced emission-line nebulosity and star formation in the high-redshift radio galaxy 4C 41.17 GV Bicknell, RS Sutherland, WJM van Breugel, MA Dopita, A Dey, ... The Astrophysical Journal 540 (2), 678, 2000 | 219 | 2000 |