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Dynamical Modeling of Galaxies and Supermassive Black Holes: Axisymmetry in Triaxial Schwarzschild Orbit Superposition Models

  • Authors: Matthew E. Quenneville, Christopher M. Liepold, and Chung-Pei Ma

2021 The Astrophysical Journal Supplement Series 254 25.

  • Provider: AAS Journals

Caption: Figure 7.

Illustration of the MBH constraints for the mock data sets described in the text. Each dashed curve represents a separate realization of the noise. In the left panel, the potential is spherical, no PSF convolution is performed, and each DF component has 5 × 108 stars. In the right panel, the model is flattened, projected stellar positions are convolved with a circular Gaussian PSF with a standard deviation of 5 pc, and each DF component has 5 × 109 stars. The 1D χ2 curves are obtained by marginalizing over Vc in the smoothed 2D χ2 landscape generated by Gaussian process regression with a squared-exponential covariance function (Pedregosa et al. 2011).

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