Characterising the surface magnetic fields of T Tauri stars with high-resolution near-infrared spectroscopy

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Table 2.

Stellar parameters.

Target ID	T_eff	log g	v sin i	References
	(K)		(km s⁻¹)
TWA 7	3300 ^(a)	4.0		Yang et al. (2008)
TWA 8A	3400 ^(a)	4.0		Yang et al. (2008)
V2247 Oph	3500 ^(a)	3.5		Donati et al. (2010)
V2058 Oph	3800 ^(a)	3.5		Manara et al. (2015)
TWA 9A	4000 ^(a)	4.0		Yang et al. (2008)
TW Hya	4075 ^(a)	4.0	4.0 ^(a)	Donati et al. (2011a)
V2129 Oph	4500 ^(a)	3.5		Donati et al. (2007)
V1121 Oph	4500 ^(b)	3.5		Weise et al. (2010)

Notes. The v sin i values are given with error bars corresponding to the 1σ confidence interval.

^(a)

Adopted from the reference in the last column.

^(b)

V1121 Oph has the same reported spectral type (K5) as V2129 Oph. For this reason, we adopt the same T_eff value than V2129 Oph.

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