Quantifying biases in orbit-superposition modelling with (non-)parametric kinematics

Open Access

Table 1.

DYNAMITE runs performed with the respective kinematic input for NGC 4550 and NGC 2768.

	Non-para., S/N = 60	GH, S/N = 60	Non-para., S/N = 150	GH, S/N = 150	Regularised non-para., S/N = 60
NGC 4550	✓	✓	✓	✓	✓
NGC 2768	✓	✓	×	×	✓
See	Sect. 5	Sect. 5	Sect. 6.3	Sect. 6.3	Appendix D

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