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Stellar kinematics using a third integral of motion: method and application on the Andromeda galaxy
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Determination of masses of the central black holes in NGC 524 and 2549 using laser guide star adaptive optics
Davor Krajnovi��, Richard M. McDermid, Michele Cappellari and Roger L. Davies Monthly Notices of the Royal Astronomical Society 399(4) 1839 (2009) https://doi.org/10.1111/j.1365-2966.2009.15415.x
Recovery of the internal orbital structure of galaxies
nmagic: a fast parallel implementation of a χ2-made-to-measure algorithm for modelling observational data
Flavio De Lorenzi, Victor P. Debattista, Ortwin Gerhard and Niranjan Sambhus Monthly Notices of the Royal Astronomical Society 376(1) 71 (2007) https://doi.org/10.1111/j.1365-2966.2007.11434.x
Potential science for the OASIS integral field spectrograph with laser guide star adaptive optics
Dynamical modelling of stars and gas in NGC 2974: determination of mass-to-light ratio, inclination and orbital structure using the Schwarzschild method
D. Krajnovic, M. Cappellari, E. Emsellem, R. M. McDermid and P. T. De Zeeuw Monthly Notices of the Royal Astronomical Society 357(4) 1113 (2005) https://doi.org/10.1111/j.1365-2966.2005.08715.x
Regularized orbit models unveiling the stellar structure and dark matter halo of the Coma elliptical NGC 4807