Polarimetry and astrometry of NIR flares as event horizon scale, dynamical probes for the mass of Sgr A*

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Table 2.

Posterior mean values of the astrometry fit.

Parameter	Posterior mean
Radius
Inclination
Position angle
Enclosed mass

Notes. The model corresponding to this set of parameters is displayed in Fig. 6 (for details of the Bayesian analysis see Appendix D).

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