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Table A.2

Stellar parameters.

ID Name SpT Teff A V L M EW[Hα] FW10%[Hα]a Accretiond Ref
(K) (mag) (L) (M) (Å) (km s-1) (Y/N)

1 TCha K0 5250 2 1.34 1.1 - 400 Y 1,2
2 RECX11 K5 4350 0.4 0.73 1.2 4.4 330 Y 3
3 RECX5 M4 3370 2.4 0.14 0.3 35 330 Y 3
4 CHXR22E M3.5 3370 4.9 0.26 0.4 - - U 4
5 ISO52 M4 3370 3 0.17 0.3 b - N 5
...

Notes.The full table is available at the CDS.

(a)

We reversed the signs of the width of the Hα line taken from Rebull et al. (2010) and Winston et al. (2009), as they list a negative value for emission and positive for absorption.

(b)

The accretion properties were derived using a full X-shooter spectrum rather than only fitting the Hα line.

(c)

The accretion properties were derived using other lines (e.g., Brγ).

(d)

’Y’ means accreting, ’N’ means nonaccreting’, and ’U’ means unknown.

Reference. 1) Alcala et al. (1995), 2) Schisano et al. (2009), 3) Lawson et al. (2004), 4) Luhman (2007), 5) Manara et al. (2016).

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