X-Shooting ULLYSES: Massive stars at low metallicity - XIII. Testing the bi-stability jump in the Large Magellanic Cloud

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Table 6

Comparison of our broadening parameters with those obtained via IACOB-BROAD (Simón-Díaz & Herrero 2014) applied to high-resolution MIKE data.

Sk −	XShootU		IACOB-BROAD		MIKE
	υ_rot sin i kms⁻¹	υ_mac kms⁻¹	v_rot sin i km s⁻¹	υ_mac km s⁻¹	line
67° 2	45	20	$46_{- 15}^{+ 10}$ $46_{ - 15}^{ + 10}$	$40_{- 20}^{+ 17}$ $40_{ - 20}^{ + 17}$	Si III λ4552
67° 78	30	20	$39_{- 29}^{+ 10}$ $39_{ - 29}^{ + 10}$	$23_{- 22}^{+ 33}$ $23_{ - 22}^{ + 33}$	Si III λ4552
70° 16	35	20	$40_{- 25}^{+ 10}$ $2340_{ - 25}^{ + 10}$	$35_{- 17}^{+ 13}$ $35_{ - 17}^{ + 13}$	Si III λ4552
68° 8	40	20	$38_{- 15}^{+ 7}$ $38_{ - 15}^{ + 7}$	$22_{- 20}^{+ 22}$ $22_{ - 20}^{ + 22}$	Si III λ4552
67° 195	30	20	$28_{- 14}^{+ 8}$ $28_{ - 14}^{ + 8}$	$28_{- 16}^{+ 14}$ $28_{ - 16}^{ + 14}$	Si II λ6347

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