Table 8: SR: 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 -0.9158 0.6332 0.9158

<4500 -2.5,-2.0 -0.2961 0.4686 0.4342

<4500 -2.0,-1.5 0.2013 0.6026 0.4545

<4500 -1.5,-1.0 0.2022 0.4808 0.3597

<4500 -1.0,-0.5 -0.4289 - 0.4289

<4500 >-0.5 - - -

4500,6500 <-2.5 -0.6448 0.5575 0.6678

4500,6500 -2.5,-2.0 -0.2419 0.3023 0.2879

4500,6500 -2.0,-1.5 -0.1947 0.3054 0.2832

4500,6500 -1.5,-1.0 -0.1968 0.2580 0.2673

4500,6500 -1.0,-0.5 0.0007 0.2260 0.1700

4500,6500 >-0.5 0.3192 0.2566 0.3300

**Table 8:** SR: 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	-0.9158	0.6332	0.9158
<4500	-2.5,-2.0	-0.2961	0.4686	0.4342
<4500	-2.0,-1.5	0.2013	0.6026	0.4545
<4500	-1.5,-1.0	0.2022	0.4808	0.3597
<4500	-1.0,-0.5	-0.4289	-	0.4289
<4500	>-0.5	-	-	-
4500,6500	<-2.5	-0.6448	0.5575	0.6678
4500,6500	-2.5,-2.0	-0.2419	0.3023	0.2879
4500,6500	-2.0,-1.5	-0.1947	0.3054	0.2832
4500,6500	-1.5,-1.0	-0.1968	0.2580	0.2673
4500,6500	-1.0,-0.5	0.0007	0.2260	0.1700
4500,6500	>-0.5	0.3192	0.2566	0.3300

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