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Table E.3.
Comparison between stellar parameters derived with VOSA and from GES (Randich et al. 2018).
| Stellar | Δ log g | ΔE(B − V) | ΔTeff | # |
|---|---|---|---|---|
| association | [dex] | [mag] | [K] | |
| All Gaia Collaboration (2018b) sources with counterpart in Randich et al. (2018) | ||||
| IC 4665 | −0.44 ± 0.60 | 0.056 | 51 ± 175 | 24 |
| NGC 2547 | −0.48 ± 0.61 | 0.040 | 362 ± 814 | 87 |
| IC 2602 | −0.22 ± 0.64 | 0.037 | 329 ± 634 | 40 |
| IC 2391 | −0.047 ± 0.44 | 0.058 | −433 ± 4401 | 23 |
| All | −0.36 ± 0.61 | 0.0477 ± 0.0093 | 206 ± 1750 | 174 |
| Sub-sample with sources considered as members after this work. | ||||
| IC 4665 | −0.33 ± 0.44 | 0.056 | 43 ± 160 | 18 |
| NGC 2547 | – | 0.040 | – | – |
| IC 2602 | 0.26 | 0.037 | 280 | 1 |
| IC 2391 | – | 0.058 | – | – |
| All | −0.303 ± 0.45 | 0.0477 ± 0.0093 | 55 ± 164 | 19 |
Notes. ‘#’ is the number of sources. ‘ΔE(B − V)’ is the difference between the excess derived in Randich et al. (2018) and the one used by us.
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