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Fig. 10

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Test of the inertia tensor method for estimating the bar angle (top panel) and the b/a axis ratio (bottom panel) for our simulated dataset. The solid black lines represent the simulated, unrestricted view of the Galactic bar for different values of Rcyllim$R_{{\rm{cyl}}}^{{\rm{lim}}}$. The solid color-coded lines show measurements for different Rcyllim$R_{{\rm{cyl}}}^{{\rm{lim}}}$ in the cone view of the Galactic bar. The dashed green line indicates the selected value of Rcyllim=1.75$R_{{\rm{cyl}}}^{{\rm{lim}}} = 1.75$ kpc used in our observational dataset. The dotted black line in both panels denotes the true value of the bar angle and axis ratio set for the ellipsoidal distribution.

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