Open Access

Table A.4.

Stellar parameters for the sample of 110 members with available photometry for the SED analysis.

Source identifier Teff log L AV tBHAC15 tSDF00
(K) (L in L) (mag) (Myr) (Myr)
Gaia DR2 6013399894569703040 3700 ± 50 0.5
Gaia DR2 6013073790593533824 2700 ± 50 0.5
Gaia DR2 6011581856393988352 2800 ± 50 0.5
Gaia DR2 6011500389453302272 3200 ± 50 0.5
Gaia DR2 6011392186336443392 3900 ± 50 0.5
Gaia DR2 6011827867821601792 2700 ± 50 1.0
Gaia DR2 6010483616079976448 3800 ± 50 0.5
Gaia DR2 5994793310284482432 2600 ± 50 1.0
Gaia DR2 5994795990344219904 2600 ± 50 0.5
Gaia DR2 5994793241564999040 3500 ± 50 1.0
Gaia DR2 5994747367001754240 3600 ± 50 0.5
Gaia DR2 5995233114932232064 3700 ± 50 0.0
Gaia DR2 5995206142536938112 2800 ± 50 0.5
Gaia DR2 5995219680274445184 3500 ± 50 0.0
Gaia DR2 5995219680274444672 3100 ± 50 0.5
Gaia DR2 5998031578183659776 2800 ± 50 0.5
Gaia DR2 5997975400009713920 2600 ± 50 0.5
Gaia DR2 5995154907858605312 3600 ± 50 0.5
Gaia DR2 5995157042469914752 2700 ± 50 0.5
Gaia DR2 5995168724780802944 3800 ± 50 0.5

Notes. This table is available in its entirey at the CDS.

We provide for each star its effective temperature and bolometric luminosity derived from the SED fit with VOSA, the extinction value for dereddening the SED, and the ages inferred from the Baraffe et al. (2015, BHAC15) and Siess et al. (2000, SDF00) models.

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