GPU-Accelerated Gravitational Lensing and Dynamical (GLaD) modeling for cosmology and galaxies

Open Access

Fig. 11.

Left: Ideal kinematic data without the bins within −0.15″ to 0.15″ with 43 bins in total. Middle: Best-fit kinematic map with $χ_{kin}^{2} = 34$ $\chi_{\mathrm{kin}}^{2} = 34$ , given the composite mass model without a BH. We do not display the best-fit kinematic map of the case with $M_{BH} = 7 \times 10^{9} M_{⊙}$ $M_{\rm BH} = 7 \times 10^9 \, M_\odot$ because they show similar fitting results. Right: Normalized residual.

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