The slope of the black-hole mass versus velocity dispersion correlation
 Tremaine, S Gebhardt, K Bender, R Bower, G Dressler, A Faber, S Filippenko, A Green, R Grillmair, C Ho, L Kormendy, J Lauer, T Magorrian, J Pinkney, J Richstone, D (26 Mar 2002)
Generating Equilibrium Dark Matter Halos: Inadequacies of the Local Maxwellian Approximation
 Kazantzidis, S Magorrian, J Moore, B (18 Sep 2003)
The Centers of Early-Type Galaxies with HST. V. New WFPC2 Photometry
 Lauer, T Faber, S Gebhardt, K Richstone, D Tremaine, S Ajhar, E Aller, M Bender, R Dressler, A Filippenko, A Green, R Grillmair, C Ho, L Kormendy, J Magorrian, J Pinkney, J Siopis, C (01 Dec 2004)
The Masses of Nuclear Black Holes in Luminous Elliptical Galaxies and Implications for the Space Density of the Most Massive Black Holes
 Lauer, T Faber, S Richstone, D Gebhardt, K Tremaine, S Postman, M Dressler, A Aller, M Filippenko, A Green, R Ho, L Kormendy, J Magorrian, J Pinkney, J (29 Jun 2006)
Evidence of a Supermassive Black Hole in the Galaxy NGC 1023 from the Nuclear Stellar Dynamics
 Bower, G Green, R Bender, R Gebhardt, K Lauer, T Magorrian, J Richstone, D Danks, A Gull, T Hutchings, J Joseph, C Kaiser, M Weistrop, D Woodgate, B Nelson, C Malumuth, E (09 Nov 2000)
Black Hole Mass Determinations From Orbit Superposition Models are Reliable
 Richstone, D Gebhardt, K Aller, M Bender, R Bower, G Dressler, A Faber, S Filippenko, A Green, R Ho, L Kormendy, J Lauer, T Magorrian, J Pinkney, J Siopis, C Tremaine, S (10 Mar 2004)
Mass profiles and anisotropies of early-type galaxies
 Magorrian, J Ballantyne, D (04 Dec 2000)
Galaxies with a Central Minimum in Stellar Luminosity Density
 Lauer, T Gebhardt, K Richstone, D Tremaine, S Bender, R Bower, G Dressler, A Faber, S Filippenko, A Green, R Grillmair, C Ho, L Kormendy, J Magorrian, J Pinkney, J Laine, S Postman, M van der Marel, R (07 Jun 2002)
Central DM density cuspiness in LSB's: a stellar kinematics approach
 Pizzella, A Corsini, E Bertola, F Coccato, L Magorrian, J Sarzi, M J., J (03 Nov 2003)
Constraining black hole masses from stellar kinematics by summing over all possible distribution functions
 Magorrian, J (08 Sep 2006)
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