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Table 2:

Offsets ($\Delta $) and scatter ($\sigma $) of the differences (raw - column) between the methods: MA$\chi $ (this work).
  ADOP NGS1 ANNSR k24
  $\Delta / \sigma$ $\Delta / \sigma$ $\Delta / \sigma$ $\Delta / \sigma$

[Fe/H]

        
MA$\chi $ -0.32 / 0.23 -0.41 / 0.29 -0.17 / 0.33 -0.34 / 0.26
k24 0.04 / 0.14 -0.07 / 0.25 0.17 / 0.27  
ANNSR -0.13 / 0.22 -0.22 / 0.23    
NGS1 0.08 / 0.17      
${T_{\rm eff}}$        
MA$\chi $ -61 / 112 80 / 132 -76 / 170 -159 / 160
k24 98 / 101 244 / 166 88 / 195  
ANNSR 1 / 114 147 / 173    
NGS1 -142 / 93      
$\log g$        
MA$\chi $ 0.51 / 0.39 0.38 / 0.43 0.63 / 0.47 0.41 / 0.48
k24 0.08 / 0.35 -0.02 / 0.42 0.26 / 0.48  
ANNSR -0.14 / 0.36 -0.27 / 0.45    
NGS1 0.09 / 0.23      

Notes. ADOP (Lee et al. 2008a), NGS1 (Lee et al. 2008a), ANNSR(Re Fiorentin et al. 2007) and k24 (Allende Prieto et al. 2006) for the entire sample of selected SEGUE stars.


Source LaTeX | All tables | In the text

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