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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