Table 5
Comparison of common O, B, and A type stars with other references.
| Reference | ΔTeff(%) | Δlog g (cm s-2) | Δ[Fe/H] (dex) | No. of Stars | Sp. Type | |||
| mean | rms | mean | rms | mean | rms | /clipped | ||
|
|
||||||||
| ELODIE 3.2 A vs. I (2009) | 1.33 | 6.32 | 0.07 | 0.25 | –0.01 | 0.21 | 293/19 | O, B, A |
| ELODIE 3.2 I (2009) | –0.84 | 3.36 | –0.05 | 0.16 | 0.01 | 0.14 | 47/6 | O, B, A |
| Valdes et al. (2004) | 1.53 | 10.02 | 0.08 | 0.47 | 0.15 | 0.55 | 86/2 | O, B, A |
| 1.53 | 10.02 | 0.01 | 0.35 | 0.02 | 0.29 | 86/2/5/18 | O, B, A | |
| Cenarro et al. (2007) | 4.33 | 12.14 | 0.17 | 0.58 | 0.23 | 0.60 | 38/1 | B, A |
| 4.33 | 12.14 | 0.03 | 0.38 | –0.01 | 0.33 | 38/1/3/9 | B, A | |
Notes. For the comparison with Valdes et al. (2004) and Cenarro et al. (2007), the statistics listed in the first line are given after excluding the temperature outliers, and the second line lists the statistics after clipping those red crosses in log g and [Fe/H] panels respectively. Numbers displayed in the column of “No. of Stars /clipped” show the clipped number in the order of Teff, log g and [Fe/H].
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