Table 6: RR: partial results. We list the mean $\mu$ and the corresponding standard deviation $\sigma$ of the difference Committee-SSPP for each of the different stellar temperatures and metallicity ranges.
$T_{\rm eff}$ ${\rm [Fe/H]}$ $\mu_{\rm [Fe/H]}$ $\sigma_{\rm [Fe/H]}$ $E_{\rm [Fe/H]}$

<4500 <-2.5 0.9062 0.8550 0.9062

<4500 -2.5,-2.0 0.2322 0.1414 0.2322

<4500 -2.0,-1.5 0.3464 0.3664 0.4503

<4500 -1.5,-1.0 0.1196 0.1779 0.1667

<4500 -1.0,-0.5 -0.1419 0.1634 0.1732

<4500 > -0.5 -0.4616 0.1322 0.4616

4500,6500 <-2.5 0.1183 0.1770 0.1574

4500,6500 -2.5,-2.0 -0.0043 0.1608 0.1144

4500,6500 -2.0,-1.5 -0.0133 0.1636 0.1219

4500,6500 -1.5,-1.0 -0.0435 0.1683 0.1303

4500,6500 -1.0,-0.5 -0.0294 0.1291 0.0999

4500,6500 >-0.5 -0.1416 0.1207 0.1456

**Table 6:** RR: partial results. We list the mean $\mu$ and the corresponding standard deviation $\sigma$ of the difference Committee-SSPP for each of the different stellar temperatures and metallicity ranges.
$T_{\rm eff}$	${\rm [Fe/H]}$	$\mu_{\rm [Fe/H]}$	$\sigma_{\rm [Fe/H]}$	$E_{\rm [Fe/H]}$
<4500	<-2.5	0.9062	0.8550	0.9062
<4500	-2.5,-2.0	0.2322	0.1414	0.2322
<4500	-2.0,-1.5	0.3464	0.3664	0.4503
<4500	-1.5,-1.0	0.1196	0.1779	0.1667
<4500	-1.0,-0.5	-0.1419	0.1634	0.1732
<4500	> -0.5	-0.4616	0.1322	0.4616
4500,6500	<-2.5	0.1183	0.1770	0.1574
4500,6500	-2.5,-2.0	-0.0043	0.1608	0.1144
4500,6500	-2.0,-1.5	-0.0133	0.1636	0.1219
4500,6500	-1.5,-1.0	-0.0435	0.1683	0.1303
4500,6500	-1.0,-0.5	-0.0294	0.1291	0.0999
4500,6500	>-0.5	-0.1416	0.1207	0.1456

Source LaTeX | All tables | In the text