The validation of made-to-measure method for reconstruction of phase space distribution functions
Hiromichi Tagawa, Naoteru Gouda, Taihei Yano, Takuji Hara

TL;DR
This paper evaluates the accuracy of the made-to-measure (M2M) method in reconstructing phase space distribution functions in galactic models, demonstrating high accuracy for spherical models and moderate for axisymmetric ones.
Contribution
It provides a detailed assessment of the M2M method's accuracy in recovering distribution functions for specific galactic models with analytic solutions.
Findings
Recovery accuracy is a few percent for spherical models.
Recovery accuracy exceeds ten percent for axisymmetric models.
The study explores parameter dependence and procedural aspects of the M2M method.
Abstract
We investigate how accurately phase space distribution functions (DFs) in galactic models can be reconstructed by a made-to-measure (M2M) method, which constructs -particle models of stellar systems from photometric and various kinematic data. The advantage of the M2M method is that this method can be applied to various galactic models without assumption of the spatial symmetries of gravitational potentials adopted in galactic models, and furthermore, numerical calculations of the orbits of the stars cannot be severely constrained by the capacities of computer memories. The M2M method has been applied to various galactic models. However, the degree of accuracy for the recovery of DFs derived by the M2M method in galactic models has never been investigated carefully. Therefore, we show the degree of accuracy for the recovery of the DFs for the anisotropic Plummer model and the…
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