Detailed lens modeling and kinematics of the submillimeter galaxy G09v1.97 - An analysis of CO, H2O, H2O+, and dust continuum emission

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Table 5.

Best-fit parametric from ^3DBAROLO fitting.

Parameter	Value
PA_kin^a	6.7
i°^b	50
V_sys^c	109
V_rot, max^d [km/s]	$388_{- 36}^{55}$ $Mathematical equation: $ 388^{55}_{-36} $$
$\bar{σ}$ $Mathematical equation: $ \bar{\sigma} $$ ^e [km/s]	$138_{- 6}^{+ 7}$ $Mathematical equation: $ 138^{+7}_{-6} $$
$V_{rot, \max} / \bar{σ}$ $Mathematical equation: $ V_{\mathrm{rot,max}}/\bar{\sigma} $$ ^f	2.8 ± 0.4

Notes.

^(a)

The position angle of the disk, measured counterclockwise from the y-axis.

^(b)

The inclination angle of the disk.

^(c)

Systemic velocity of the CO(6−5) line.

^(d)

Maximum rotation velocity across all rings.

^(e)

Average σ value across all rings.

^(f)

Ratio of the maximum rotational velocity over the average σ with errors propagated.

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