<table><caption>**Table 11.** Summary of element abundance detections (D) and lines measured (L).</caption><thead><tr><th rowspan="2">Species</th><th colspan="3">HR10 (D,L)</th><th colspan="3">HR21 (D,L)</th><th colspan="3">HR15N (D,L)</th><th colspan="2">HR9B (D,L)</th><th rowspan="2">WG11</th><th rowspan="2">X-Match</th><th rowspan="2">References</th></tr><tr><th>Lumba</th><th>CAUP</th><th>Vilnius</th><th>Lumba</th><th>CAUP</th><th>Vilnius</th><th>EPINARBO</th><th>Lumba</th><th>CAUP</th><th>EPINARBO</th></tr></thead><tbody><tr><td>AL1</td><td>—,—</td><td>—,—</td><td>10 173,2</td><td>27 068,1</td><td>23 983,2</td><td>32 238,2</td><td>9057,2</td><td>6021,2</td><td>—,—</td><td>—,—</td><td>—,—</td><td>555</td><td>Wiese et al. (1969)</td></tr><tr><td>BA2</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>1008,1</td><td>11 946,1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>553</td><td>Miles &amp; Wiese (1969)</td></tr><tr><td>C1</td><td>634,1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>5536,1</td><td>1779,1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>460</td><td>Kurucz (2010); Ralchenko et al. (2010)</td></tr><tr><td>CA1</td><td>—,—</td><td>3065,1</td><td>33 719,6</td><td>—,—</td><td>—,—</td><td>—,—</td><td>6561,2</td><td>12 667,3</td><td>4758,1</td><td>—,—</td><td>—,—</td><td>583</td><td>Smith (1981, 1988); Smith &amp; Raggett (1981)</td></tr><tr><td>CA2</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>40 787,3</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>318</td><td>Theodosiou (1989); Seaton et al. (1994)</td></tr><tr><td>CE2</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>686,2</td><td>387</td><td>Lawler et al. (2009)</td></tr><tr><td>CO1</td><td>2883,1</td><td>300,1</td><td>21 164,6</td><td>—,—</td><td>—,—</td><td>—,—</td><td>9139,2</td><td>4854,2</td><td>—,—</td><td>—,—</td><td>—,—</td><td>575</td><td>Kurucz (2008)</td></tr><tr><td>CR1</td><td>17 040,2</td><td>11 275,2</td><td>39 180,6</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>582</td><td>Wallace &amp; Hinkle (2009)</td></tr><tr><td>CR2</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>205,1</td><td>Pinnington et al. (1993)</td></tr><tr><td>CU1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>572</td><td>Kurucz (2012)</td></tr><tr><td>DY2</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>75,1</td><td>Wickliffe et al. (2000)</td></tr><tr><td>EU2</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>474</td><td>Lawler et al. (2001b)</td></tr><tr><td>FE1</td><td>35 301,16</td><td>22 137,3</td><td>40 969,28</td><td>28 165,7</td><td>20 606,2</td><td>44 674,7</td><td>9263,18</td><td>—,—</td><td>7117,4</td><td>—,—</td><td>—,—</td><td>580</td><td>Fuhr et al. (1988); Bard &amp; Kock (1994); Kurucz (2007); O'Brian et al. (1991)</td></tr><tr><td>FE2</td><td>—,—</td><td>—,—</td><td>24 823,2</td><td>—,—</td><td>—,—</td><td>—,—</td><td>8918,2</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>563</td><td>Kurucz (2013)</td></tr><tr><td>LA2</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>316</td><td>Lawler et al. (2001a)</td></tr><tr><td>LI1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>4905,1</td><td>319,1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>548</td><td>Lindgård &amp; Nielson (1977)</td></tr><tr><td>MG1</td><td>17 542,1</td><td>—,—</td><td>41 162,2</td><td>24 751,2</td><td>40 834,2</td><td>44 250,3</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>2,2</td><td>569</td><td>Kurucz &amp; Peytremann (1975); Ralchenko et al. (2010)</td></tr><tr><td>MN1</td><td>12 838,2</td><td>2745,1</td><td>33 859,4</td><td>—,—</td><td>—,—</td><td>—,—</td><td>6,1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>550</td><td>Kurucz (2007)</td></tr><tr><td>MO2</td><td>198,1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>222</td><td>Whaling &amp; Brault (1988)</td></tr><tr><td>ND2</td><td>736,1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>3493,1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>567</td><td>Den Hartog et al. (2003); Meggers et al. (1975)</td></tr><tr><td>NI1</td><td>4265,2</td><td>570,1</td><td>34 672,5</td><td>—,—</td><td>—,—</td><td>—,—</td><td>8978,3</td><td>9961,4</td><td>4417,2</td><td>—,—</td><td>—,—</td><td>579</td><td>Kurucz (2008); Wickliffe &amp; Lawler (1997)</td></tr><tr><td>PR2</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>234</td><td>Ivarsson et al. (2001); Biémont et al. (2003)</td></tr><tr><td>S1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>7733,2</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>218</td><td>Biemont et al. (1993); Kurucz (2004)</td></tr><tr><td>SC2</td><td>14 039,1</td><td>616,1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>9063,1</td><td>—,—</td><td>2937,1</td><td>—,—</td><td>—,—</td><td>575</td><td>Lawler &amp; Dakin (1989)</td></tr><tr><td>SI1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>9219,1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>575</td><td>Kurucz (2007); Garz (1973)</td></tr><tr><td>SR1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>3516,1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—</td><td>García &amp; Campos (1988)</td></tr><tr><td>TI1</td><td>—,—</td><td>—,—</td><td>31 799,7</td><td>—,—</td><td>—,—</td><td>18 235,2</td><td>9027,2</td><td>7878,2</td><td>—,—</td><td>—,—</td><td>—,—</td><td>584</td><td>Kurucz (2010); Nitz et al. (1998); Lawler et al. (2013)</td></tr><tr><td>TI2</td><td>—,—</td><td>511,1</td><td>35 712,6</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>575</td><td>Wood et al. (2013)</td></tr><tr><td>V1</td><td>2209,1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>7321,1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>575</td><td>Kurucz (2009)</td></tr><tr><td>Y2</td><td>406,2</td><td>—,—</td><td>5647,2</td><td>—,—</td><td>—,—</td><td>—,—</td><td>4117,1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>571</td><td>Pitts &amp; Newsom (1986); Kurucz (2011); Biémont et al. (2011); Hannaford et al. (1982)</td></tr><tr><td>ZR1</td><td>243,1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>84,1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>399</td><td>Biemont et al. (1981)</td></tr></tbody></table>

**Notes.** Summary per node per SETUP of the number of CNAMEs that have abundance detections (D) and average number of spectral lines measured per species (L). The number of CNAMEs in the cross-match with all WG10 SETUPs for which each abundance is measured by WG11.

<table><caption>**Table 12.** Element measurements rejection criteria.</caption><thead><tr><th>SETUP</th><th>ELEMENT</th><th>Crit.</th></tr></thead><tbody><tr><td>HR15N</td><td>AL1</td><td>>10</td></tr><tr><td>HR15N</td><td>CO1</td><td>>7</td></tr><tr><td>HR15N</td><td>EU2</td><td>>4</td></tr><tr><td>HR15N</td><td>NI1</td><td>>8</td></tr><tr><td>HR15N</td><td>NI1</td><td>&lt;2</td></tr><tr><td>HR15N</td><td>TI1</td><td>>9</td></tr><tr><td>HR15N</td><td>TI1</td><td>&lt;2</td></tr><tr><td>HR10</td><td>C1</td><td>>10</td></tr><tr><td>HR10</td><td>MO1</td><td>>4</td></tr><tr><td>HR10</td><td>V1</td><td>>5</td></tr><tr><td>HR10</td><td>Y2</td><td>>5</td></tr><tr><td>HR21</td><td>MG1</td><td>>15</td></tr><tr><td>HR21</td><td>SI1</td><td>>20</td></tr></tbody></table>

**Notes.** Elements for specific SETUPs and Node analyses for which extrema in absolute abundance were rejected if above (>) or below (<) the rejection criteria (Crit.) threshold.

<table><caption>**Table 13.** Set of corrections calculated for each parameter for each ELEMENT+SETUP+NODE combination.</caption><tbody><tr><td>1</td><td>Median and standard deviation of the difference</td></tr><tr><td>2</td><td>Linear fit to the difference against<br/>a) FEH<br/>b) TEFF<br/>c) LOGG</td></tr><tr><td>3</td><td>Quadratic fit to the difference against<br/>a) FEH<br/>b) TEFF<br/>c) LOGG</td></tr></tbody></table>

points in Fig. 14). The set was then divided into ten evenly distributed bins spanning the range of the reference values for the respective parameter ($T_{eff}$, log g, or [Fe/H]). The median and
<table><caption>**Table 11.** Summary of element abundance detections (D) and lines measured (L).</caption><thead><tr><th rowspan="2">Species</th><th colspan="3">HR10 (D,L)</th><th colspan="3">HR21 (D,L)</th><th colspan="3">HR15N (D,L)</th><th colspan="3">HR9B (D,L)</th><th rowspan="2">WG11</th><th rowspan="2">X-Match</th><th rowspan="2">References</th></tr><tr><th>Lumba</th><th>CAUP</th><th>Vilnius</th><th>Lumba</th><th>CAUP</th><th>Vilnius</th><th>EPINARBO</th><th>Lumba</th><th>CAUP</th><th>EPINARBO</th><th>Lumba</th><th>CAUP</th><th>EPINARBO</th></tr></thead><tbody><tr><td>AL1</td><td>—,—</td><td>—,—</td><td>10 173,2</td><td>27 068,1</td><td>23 983,2</td><td>32 238,2</td><td>9057,2</td><td>6021,2</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>555</td><td>Wiese et al. (1969)</td></tr><tr><td>BA2</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>1008,1</td><td>11 946,1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>553</td><td>Miles &amp; Wiese (1969)</td></tr><tr><td>C1</td><td>634,1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>5536,1</td><td>1779,1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>460</td><td>Kurucz (2010); Ralchenko et al. (2010)</td></tr><tr><td>CA1</td><td>—,—</td><td>3065,1</td><td>33 719,6</td><td>—,—</td><td>—,—</td><td>—,—</td><td>6561,2</td><td>12 667,3</td><td>4758,1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>583</td><td>Smith (1981, 1988); Smith &amp; Raggett (1981)</td></tr><tr><td>CA2</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>40 787,3</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>318</td><td>Theodosiou (1989); Seaton et al. (1994)</td></tr><tr><td>CE2</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>387</td><td>Lawler et al. (2009)</td></tr><tr><td>CO1</td><td>2883,1</td><td>300,1</td><td>21 164,6</td><td>—,—</td><td>—,—</td><td>—,—</td><td>9139,2</td><td>4854,2</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>575</td><td>Kurucz (2008)</td></tr><tr><td>CR1</td><td>17 040,2</td><td>11 275,2</td><td>39 180,6</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>582</td><td>Wallace &amp; Hinkle (2009)</td></tr><tr><td>CR2</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>205,1</td><td>Pinnington et al. (1993)</td></tr><tr><td>CU1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>368,1</td><td>Kurucz (2012)</td></tr><tr><td>DY2</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>75,1</td><td>Wickliffe et al. (2000)</td></tr><tr><td>EU2</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>474</td><td>Lawler et al. (2001b)</td></tr><tr><td>FE1</td><td>35 301,16</td><td>22 137,3</td><td>40 969,28</td><td>28 165,7</td><td>20 606,2</td><td>44 674,7</td><td>9263,18</td><td>—,—</td><td>7117,4</td><td>—,—</td><td>—,—</td><td>—,—</td><td>580</td><td>Fuhr et al. (1988); Bard &amp; Kock (1994); Kurucz (2007); O'Brian et al. (1991)</td></tr><tr><td>FE2</td><td>—,—</td><td>—,—</td><td>24 823,2</td><td>—,—</td><td>—,—</td><td>—,—</td><td>8918,2</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>563</td><td>Kurucz (2013)</td></tr><tr><td>LA2</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>316</td><td>Lawler et al. (2001a)</td></tr><tr><td>LI1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>4905,1</td><td>319,1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>548</td><td>Lindgård &amp; Nielson (1977)</td></tr><tr><td>MG1</td><td>17 542,1</td><td>—,—</td><td>41 162,2</td><td>24 751,2</td><td>40 834,2</td><td>44 250,3</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>569</td><td>Kurucz &amp; Peytremann (1975); Ralchenko et al. (2010)</td></tr><tr><td>MN1</td><td>12 838,2</td><td>2745,1</td><td>33 859,4</td><td>—,—</td><td>—,—</td><td>—,—</td><td>6,1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>550</td><td>Kurucz (2007)</td></tr><tr><td>MO2</td><td>198,1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>222</td><td>Whaling &amp; Brault (1988)</td></tr><tr><td>ND2</td><td>736,1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>3493,1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>567</td><td>Den Hartog et al. (2003); Meggers et al. (1975)</td></tr><tr><td>NI1</td><td>4265,2</td><td>570,1</td><td>34 672,5</td><td>—,—</td><td>—,—</td><td>—,—</td><td>8978,3</td><td>9961,4</td><td>4417,2</td><td>—,—</td><td>—,—</td><td>—,—</td><td>579</td><td>Kurucz (2008); Wickliffe &amp; Lawler (1997)</td></tr><tr><td>PR2</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>234</td><td>Ivarsson et al. (2001); Biémont et al. (2003)</td></tr><tr><td>S1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>7733,2</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>218</td><td>Biemont et al. (1993); Kurucz (2004)</td></tr><tr><td>SC2</td><td>14 039,1</td><td>616,1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>9063,1</td><td>—,—</td><td>2937,1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>575</td><td>Lawler &amp; Dakin (1989)</td></tr><tr><td>SI1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>9219,1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>575</td><td>Kurucz (2007); Garz (1973)</td></tr><tr><td>SR1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>3516,1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—</td><td>García &amp; Campos (1988)</td></tr><tr><td>TI1</td><td>—,—</td><td>—,—</td><td>31 799,7</td><td>—,—</td><td>—,—</td><td>18 235,2</td><td>9027,2</td><td>7878,2</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>584</td><td>Kurucz (2010); Nitz et al. (1998); Lawler et al. (2013)</td></tr><tr><td>TI2</td><td>—,—</td><td>511,1</td><td>35 712,6</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>884,2</td><td>Wood et al. (2013)</td></tr><tr><td>V1</td><td>2209,1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>7321,1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>575</td><td>Kurucz (2009)</td></tr><tr><td>Y2</td><td>406,2</td><td>—,—</td><td>5647,2</td><td>—,—</td><td>—,—</td><td>—,—</td><td>4117,1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>571</td><td>Pitts &amp; Newsom (1986); Kurucz (2011); Biémont et al. (2011); Hannaford et al. (1982)</td></tr><tr><td>ZR1</td><td>243,1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>84,1</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>—,—</td><td>399</td><td>Biemont et al. (1981)</td></tr></tbody></table>

**Notes.** Summary per node per SETUP of the number of CNAMEs that have abundance detections (D) and average number of spectral lines measured per species (L). The number of CNAMEs in the cross-match with all WG10 SETUPs for which each abundance is measured by WG11.

<table><caption>**Table 12.** Element measurements rejection criteria.</caption><thead><tr><th>SETUP</th><th>ELEMENT</th><th>Crit.</th></tr></thead><tbody><tr><td>HR15N</td><td>AL1</td><td>>10</td></tr><tr><td>HR15N</td><td>CO1</td><td>>7</td></tr><tr><td>HR15N</td><td>EU2</td><td>>4</td></tr><tr><td>HR15N</td><td>NI1</td><td>>8</td></tr><tr><td>HR15N</td><td>NI1</td><td>&lt;2</td></tr><tr><td>HR15N</td><td>TI1</td><td>>9</td></tr><tr><td>HR15N</td><td>TI1</td><td>&lt;2</td></tr><tr><td>HR10</td><td>C1</td><td>>10</td></tr><tr><td>HR10</td><td>MO1</td><td>>4</td></tr><tr><td>HR10</td><td>V1</td><td>>5</td></tr><tr><td>HR10</td><td>Y2</td><td>>5</td></tr><tr><td>HR21</td><td>MG1</td><td>>15</td></tr><tr><td>HR21</td><td>SI1</td><td>>20</td></tr></tbody></table>

**Notes.** Elements for specific SETUPs and Node analyses for which extrema in absolute abundance were rejected if above (>) or below (<) the rejection criteria (Crit.) threshold.

<table><caption>**Table 13.** Set of corrections calculated for each parameter for each ELEMENT+SETUP+NODE combination.</caption><tbody><tr><td>1</td><td>Median and standard deviation of the difference</td></tr><tr><td>2</td><td>Linear fit to the difference against<br/>a) FEH<br/>b) TEFF<br/>c) LOGG</td></tr><tr><td>3</td><td>Quadratic fit to the difference against<br/>a) FEH<br/>b) TEFF<br/>c) LOGG</td></tr></tbody></table>

points in Fig. 14). The set was then divided into ten evenly distributed bins spanning the range of the reference values for the respective parameter ($T_{eff}$, log g, or [Fe/H]). The median and
<figure><img src="image_14.png" /><figcaption>**Fig. 14.** Difference between node values and reference values in example case of the CAUP analysis of Mg I measured in the HR21 spectrum. Top row: differences against [Fe/H] for the full sample (left-black), the giants (middle-red), and the dwarfs (right-blue). Middle row: same but against log g. Bottom row: same but against T<sub>eff</sub>. The differences as median differences calculated per bins are shown as orange points with error bars. The linear fit (orange dot-dash) and quadratic fit (red dot-dash) are shown in each case.</figcaption></figure>

<table><caption>**Table 14.** Abundance corrections derived using the full WG11 dataset.</caption><thead><tr><th>Setup</th><th>Node</th><th>Element</th></tr></thead><tbody><tr><td>HR10</td><td>Lumba</td><td>MO1</td></tr><tr><td>HR10</td><td>Lumba</td><td>ZR1</td></tr><tr><td>HR15N</td><td>EPINARBO</td><td>BA2</td></tr><tr><td>HR15N</td><td>EPINARBO</td><td>ND2</td></tr><tr><td>HR15N</td><td>EPINARBO</td><td>ZR1</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>CR2</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>CU1</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>LA2</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>PR2</td></tr></tbody></table>

**Notes.** List of SETUP+NODE+ELEMENT combinations for which the sample was compared to the full W11 dataset for deriving the correction relation, WG11-full.

standard deviation of the differences in each bin were then calculated (orange points with error bars in Fig. 14). The median difference and standard deviation, linear fit, and quadratic fit to the binned data points were then calculated (shown as orange dot-dashed line and red dot-dashed line, respectively in Fig. 14). The coefficients and goodness of fit for the range of corrections were returned and examined.

Table B.1 gives the coefficients of the fit and the parameter range for the final set of corrections. While useful numbers with which to derive a correction were returned for the majority of SETUP+NODE+ELEMENT combinations (indicated as WG11xmat in the 'Calibration' column of the table), there were nonetheless cases for which there were not enough data points with which to work.

<table><caption>**Table 15.** Abundance corrections derived using the solar chemical composition.</caption><thead><tr><th>Setup</th><th>Node</th><th>Element</th></tr></thead><tbody><tr><td>HR15N</td><td>EPINARBO</td><td>SR1</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>DY2</td></tr></tbody></table>

**Notes.** List of SETUP+NODE+ELEMENT combinations for which the sample was compared to the solar chemical abundance for deriving the correction offset, Scaled Solar.

<table><caption>**Table 16.** Extreme abundance enhancement present at super-solar metallicity.</caption><thead><tr><th>Setup</th><th>Node</th><th>Element</th></tr></thead><tbody><tr><td>HR21</td><td>CAUP</td><td>FE1</td></tr><tr><td>HR21</td><td>Lumba</td><td>FE1</td></tr><tr><td>HR21</td><td>Vilnius</td><td>CA2</td></tr><tr><td>HR21</td><td>Vilnius</td><td>FE1</td></tr><tr><td>HR21</td><td>Vilnius</td><td>MG1</td></tr><tr><td>HR21</td><td>Vilnius</td><td>TI1</td></tr></tbody></table>

**Notes.** List of SETUP+NODE+ELEMENT combinations for which the sample showed an upturn at super-solar [Fe/H] in HR21 but not in HR10, HR21toHR10-WG11.

There were three exceptions to the general case: (1) Insufficient element abundances in the WG11 cross-match sample but a reasonably useful number in the rest of the WG11 dataset (WG11-full). (2) No WG11 abundances at all for that element
<figure><img src="image_15.png" /><figcaption>**Fig. 14.** Difference between node values and reference values in example case of the CAUP analysis of Mg I measured in the HR21 spectrum. Top row: differences against [Fe/H] for the full sample (left-black), the giants (middle-red), and the dwarfs (right-blue). Middle row: same but against log g. Bottom row: same but against $T_{eff}$. The differences as median differences calculated per bins are shown as orange points with error bars. The linear fit (orange dot-dash) and quadratic fit (red dot-dash) are shown in each case.</figcaption></figure>

<table><caption>**Table 14.** Abundance corrections derived using the full WG11 dataset.</caption><thead><tr><th>Setup</th><th>Node</th><th>Element</th></tr></thead><tbody><tr><td>HR10</td><td>Lumba</td><td>MO1</td></tr><tr><td>HR10</td><td>Lumba</td><td>ZR1</td></tr><tr><td>HR15N</td><td>EPINARBO</td><td>BA2</td></tr><tr><td>HR15N</td><td>EPINARBO</td><td>ND2</td></tr><tr><td>HR15N</td><td>EPINARBO</td><td>ZR1</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>CR2</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>CU1</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>LA2</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>PR2</td></tr></tbody></table>

**Notes.** List of SETUP+NODE+ELEMENT combinations for which the sample was compared to the full W11 dataset for deriving the correction relation, WG11-full.

standard deviation of the differences in each bin were then calculated (orange points with error bars in Fig. 14). The median difference and standard deviation, linear fit, and quadratic fit to the binned data points were then calculated (shown as orange dot-dashed line and red dot-dashed line, respectively in Fig. 14). The coefficients and goodness of fit for the range of corrections were returned and examined.

Table B.1 gives the coefficients of the fit and the parameter range for the final set of corrections. While useful numbers with which to derive a correction were returned for the majority of SETUP+NODE+ELEMENT combinations (indicated as WG11xmat in the 'Calibration' column of the table), there were nonetheless cases for which there were not enough data points with which to work.

<table><caption>**Table 15.** Abundance corrections derived using the solar chemical composition.</caption><thead><tr><th>Setup</th><th>Node</th><th>Element</th></tr></thead><tbody><tr><td>HR15N</td><td>EPINARBO</td><td>SR1</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>DY2</td></tr></tbody></table>

**Notes.** List of SETUP+NODE+ELEMENT combinations for which the sample was compared to the solar chemical abundance for deriving the correction offset, Scaled Solar.

<table><caption>**Table 16.** Extreme abundance enhancement present at super-solar metallicity.</caption><thead><tr><th>Setup</th><th>Node</th><th>Element</th></tr></thead><tbody><tr><td>HR21</td><td>CAUP</td><td>FE1</td></tr><tr><td>HR21</td><td>Lumba</td><td>FE1</td></tr><tr><td>HR21</td><td>Vilnius</td><td>CA2</td></tr><tr><td>HR21</td><td>Vilnius</td><td>FE1</td></tr><tr><td>HR21</td><td>Vilnius</td><td>MG1</td></tr><tr><td>HR21</td><td>Vilnius</td><td>TI1</td></tr></tbody></table>

**Notes.** List of SETUP+NODE+ELEMENT combinations for which the sample showed an upturn at super-solar [Fe/H] in HR21 but not in HR10, HR21toHR10-WG11.

There were three exceptions to the general case: (1) Insufficient element abundances in the WG11 cross-match sample but a reasonably useful number in the rest of the WG11 dataset (WG11-full). (2) No WG11 abundances at all for that element
<figure><img src="image_15.png" /><figcaption>**Fig. 15.** Comparing HR21 (by cross-match) with HR10 uncorrected (HR10uncor), HR10 corrected to WG11 (HR10cor), and WG11. Top row: the bulge sample (BL); Middle row: the giant sample (GT); bottom row: the dwarf sample (DW). First column: Ti I abundances against [Fe/H]; second column: difference between HR21 and HR10 abundances (HR10uncor and HR10cor) with linear, quadratic and cubic fits; third column: application of correction from quadratic fit to HR21 (HR21cor).</figcaption></figure>

(Scaled Solar). (3) Super-solar trend in HR21 compared to HR10 (HR21toHR10-WG11).

In the first case, there were nine SETUP+NODE+ ELEMENT combinations for which the full WG11 element abundance distribution was used to estimate a correction. These combinations are listed in Table 14.

In the second case, there were two combinations for which the only option was to scale to the solar abundance. These two combinations are listed in Table 15.

In the third case, comparison of the HR21 BL to HR10 BL abundances revealed an exaggerated upturning to enhanced abundances at the metal-rich end. Further exploration showed that this was a difference between the giants and dwarfs. The dwarf sample did not show this in neither HR21 nor HR10. This upturning seemed extreme for an astrophysical effect, but it could not be compared to the reference sample as there were no stars in common between HR21 and WG11 for the bulge sample.

However, there was the cross-match sample between HR21 and HR10 to examine. The equivalent set in HR10 did not show such an extreme upturning at the metal-rich end, though for some abundances it was slightly present which could indicate an astrophysical effect. The goal was to put giants in HR21 onto the same scale as giants in HR10 but not to remove the feature completely if present in both sets of results.

Thus HR21 giants cross-matched to the HR10 giants sample were used to remove any systematic without erasing a

potential astrophysical signature. However, just because the giants in HR21 behaved differently compared to the dwarfs in HR21, this did not necessarily mean that the dwarfs in HR21 behaved the same as those in HR10. It was necessary to investigate a correction to HR10 for the dwarf targets in HR21 to also ensure all targets were put onto the HR10 scale. As HR10 was corrected onto the WG11 scale separately, this was carried out first. Then HR21 was corrected onto HR10, which had already been corrected onto the WG11 scale. The SETUP+NODE+ELEMENT combinations for which the corrections needed to be calculated are listed in Table 16.

Figure 15 illustrates the process of determining and applying the correction using the Vilnius and Ti I results as an example. The panels show the Ti I abundances against [Fe/H], comparing HR21 with the uncorrected HR10 (HR10uncor), HR10 corrected to WG11 (HR10cor), and WG11. The first row shows the cross-match to HR10 for the bulge sample (BL), the second row shows the giant sample (GT) and the third row shows the dwarf sample (DW). The first column shows HR21 uncorrected. The upturn at super solar is clear in the HR21 giant sample (we note that the bulge stars are also giants) when compared to the HR10 giant sample, the dwarfs in both HR21 and HR10, and WG11. The second column shows the linear, quadratic and cubic fit to the difference in Ti I values of the cross-match between HR21 and HR10uncor and HR10cor for the bulge, giants, and dwarfs. The third column applies the correction from the quadratic fit to the HR21 values in each case. The procedure successfully scales
<figure><img src="image_16.png" /><figcaption>**Fig. 15.** Comparing HR21 (by cross-match) with HR10 uncorrected (HR10uncor), HR10 corrected to WG11 (HR10cor), and WG11. Top row: the bulge sample (BL); Middle row: the giant sample (GT); bottom row: the dwarf sample (DW). First column: Ti I abundances against [Fe/H]; second column: difference between HR21 and HR10 abundances (HR10uncor and HR10cor) with linear, quadratic and cubic fits; third column: application of correction from quadratic fit to HR21 (HR21cor).</figcaption></figure>

(Scaled Solar). (3) Super-solar trend in HR21 compared to HR10 (HR21toHR10-WG11).

In the first case, there were nine SETUP+NODE+ ELEMENT combinations for which the full WG11 element abundance distribution was used to estimate a correction. These combinations are listed in Table 14.

In the second case, there were two combinations for which the only option was to scale to the solar abundance. These two combinations are listed in Table 15.

In the third case, comparison of the HR21 BL to HR10 BL abundances revealed an exaggerated upturning to enhanced abundances at the metal-rich end. Further exploration showed that this was a difference between the giants and dwarfs. The dwarf sample did not show this in neither HR21 nor HR10. This upturning seemed extreme for an astrophysical effect, but it could not be compared to the reference sample as there were no stars in common between HR21 and WG11 for the bulge sample.

However, there was the cross-match sample between HR21 and HR10 to examine. The equivalent set in HR10 did not show such an extreme upturning at the metal-rich end, though for some abundances it was slightly present which could indicate an astrophysical effect. The goal was to put giants in HR21 onto the same scale as giants in HR10 but not to remove the feature completely if present in both sets of results.

Thus HR21 giants cross-matched to the HR10 giants sample were used to remove any systematic without erasing a

potential astrophysical signature. However, just because the giants in HR21 behaved differently compared to the dwarfs in HR21, this did not necessarily mean that the dwarfs in HR21 behaved the same as those in HR10. It was necessary to investigate a correction to HR10 for the dwarf targets in HR21 to also ensure all targets were put onto the HR10 scale. As HR10 was corrected onto the WG11 scale separately, this was carried out first. Then HR21 was corrected onto HR10, which had already been corrected onto the WG11 scale. The SETUP+NODE+ELEMENT combinations for which the corrections needed to be calculated are listed in Table 16.

Figure 15 illustrates the process of determining and applying the correction using the Vilnius and Ti I results as an example. The panels show the Ti I abundances against [Fe/H], comparing HR21 with the uncorrected HR10 (HR10uncor), HR10 corrected to WG11 (HR10cor), and WG11. The first row shows the cross-match to HR10 for the bulge sample (BL), the second row shows the giant sample (GT) and the third row shows the dwarf sample (DW). The first column shows HR21 uncorrected. The upturn at super solar is clear in the HR21 giant sample (we note that the bulge stars are also giants) when compared to the HR10 giant sample, the dwarfs in both HR21 and HR10, and WG11. The second column shows the linear, quadratic and cubic fit to the difference in Ti I values of the cross-match between HR21 and HR10uncor and HR10cor for the bulge, giants, and dwarfs. The third column applies the correction from the quadratic fit to the HR21 values in each case. The procedure successfully scales
<figure><img src="image_16.png" /><figcaption>**Fig. 16.** Errors on WG10-recommended abundances (in absolute abundance) against S/N on a log scale. Sub-samples per NN are shown as specified in the top-left panel.</figcaption></figure>

HR21 and HR10 to WG11 while retaining any subtle potentially astrophysical effects.

### 7.4. Errors in the homogenised abundances

Figure 16 shows the error distributions against S/N for the homogenised WG10 abundances. For the LbL abundances, the error in the abundances was calculated as the standard deviation of the set of node LbL abundances used per target in the homogenisation. In some cases if a single line abundance from a single node was the only abundance available, then the error provided by that node was reported as the error.

There were three situations in which errors would potentially end up missing from the final homogenisation: (1) No error was provided with the single line abundance measurement although errors for other measurements for the same element for that node were provided. (2) No errors were provided at all by

the node for the LbL abundances of that element. (3) No errors were provided at all by the node for the LbL abundances of any element.

Three relations were derived to complete the final errors. (1) An error relation with S/N was generated for each NODE+SETUP+ELEMENT combination. (2) An error relation with S/N was generated by combining all reported errors for all abundances provided by the node for the SETUP. (3) For each CNAME and SETUP, the spread in each abundance that had more than one line was calculated across the node values and was used to calculate an uncertainty relation with S/N per abundance per SETUP.

Thus, in the homogenisation procedure, if the final abundance was based on a single node value that did not have an associated error, the appropriate relation was used to provide an estimate of the uncertainty, which was then reported as the final error on that abundance. In this way, all values in the
<figure><img src="image_17.png" /><figcaption>**Fig. 16.** Errors on WG10-recommended abundances (in absolute abundance) against S/N on a log scale. Sub-samples per NN are shown as specified in the top-left panel.</figcaption></figure>

HR21 and HR10 to WG11 while retaining any subtle potentially astrophysical effects.

### 7.4. Errors in the homogenised abundances

Figure 16 shows the error distributions against S/N for the homogenised WG10 abundances. For the LbL abundances, the error in the abundances was calculated as the standard deviation of the set of node LbL abundances used per target in the homogenisation. In some cases if a single line abundance from a single node was the only abundance available, then the error provided by that node was reported as the error.

There were three situations in which errors would potentially end up missing from the final homogenisation: (1) No error was provided with the single line abundance measurement although errors for other measurements for the same element for that node were provided. (2) No errors were provided at all by

the node for the LbL abundances of that element. (3) No errors were provided at all by the node for the LbL abundances of any element.

Three relations were derived to complete the final errors. (1) An error relation with S/N was generated for each NODE+SETUP+ELEMENT combination. (2) An error relation with S/N was generated by combining all reported errors for all abundances provided by the node for the SETUP. (3) For each CNAME and SETUP, the spread in each abundance that had more than one line was calculated across the node values and was used to calculate an uncertainty relation with S/N per abundance per SETUP.

Thus, in the homogenisation procedure, if the final abundance was based on a single node value that did not have an associated error, the appropriate relation was used to provide an estimate of the uncertainty, which was then reported as the final error on that abundance. In this way, all values in the
<figure><img src="image_17.png" /><figcaption>**Fig. 17.** Final WG10 abundances against WG11 abundances for the CNAMEs in common with WG11 for each WG10 homogenised element. The median difference and spread are provided for each element.</figcaption></figure>

<figure><img src="image_18.png" /><figcaption>**Fig. 18.** Final WG10 stellar parameters with S/N≥25 and NN≥2 as a) Kiel diagram with metallicity colour map, and b) Metallicity distribution.</figcaption></figure>
<figure><img src="image_18.png" /><figcaption>**Fig. 17.** Final WG10 abundances against WG11 abundances for the CNAMEs in common with WG11 for each WG10 homogenised element. The median difference and spread are provided for each element.</figcaption></figure>

<figure><img src="image_19.png" /><figcaption>**Fig. 18.** Final WG10 stellar parameters with S/N≥25 and NN≥2 as a) Kiel diagram with metallicity colour map, and b) Metallicity distribution.</figcaption></figure>
<figure><img src="image_19.png" /><figcaption>**Fig. 19.** Final WG10 chemical abundances as [X/Fe] against [Fe/H] illustrating the process of selecting by the NN contributing to the final abundance.</figcaption></figure>

WG10 abundance homogenisation have associated error values as shown in Fig. 16.

However, we observed some extreme outliers and large spread in error values for some elements. Figure 16 shows the errors by sub-sample of NN, in which the lowest errors and highest S/N are typically represented by the maximum NN sub-sample. The highest errors typically occur when less than three node results are combined. In particular, when (and despite the fact that) the S/N is high (~100), the homogenised error is also high (> 2), such as for MG1, SI1, TI1, and FE1. This may not just be attributed to a better result by combining more nodes, but also to differences in the level of data quality for which nodes

reported results. A consistent error model imposed across the nodes would have improved the resulting dataset.

### 7.5. Verification of the Working Group 10 homogenised chemical abundances

The reference set used for the calibration of the WG10 chemical abundances was the cross-match with WG11 as described in Sect. 7.3. Detailed quality checks on the WG10 homogenisation regarding key sub-samples in the context of the full survey have been carried out in Hourihane et al. (2023). In this work, we only inspect the comparison to WG11 in Fig. 17.
<figure><img src="image_20.png" /><figcaption>**Fig. 19.** Final WG10 chemical abundances as [X/Fe] against [Fe/H] illustrating the process of selecting by the NN contributing to the final abundance.</figcaption></figure>

WG10 abundance homogenisation have associated error values as shown in Fig. 16.

However, we observed some extreme outliers and large spread in error values for some elements. Figure 16 shows the errors by sub-sample of NN, in which the lowest errors and highest S/N are typically represented by the maximum NN sub-sample. The highest errors typically occur when less than three node results are combined. In particular, when (and despite the fact that) the S/N is high (~100), the homogenised error is also high (> 2), such as for MG1, SI1, TI1, and FE1. This may not just be attributed to a better result by combining more nodes, but also to differences in the level of data quality for which nodes

reported results. A consistent error model imposed across the nodes would have improved the resulting dataset.

### 7.5. Verification of the Working Group 10 homogenised chemical abundances

The reference set used for the calibration of the WG10 chemical abundances was the cross-match with WG11 as described in Sect. 7.3. Detailed quality checks on the WG10 homogenisation regarding key sub-samples in the context of the full survey have been carried out in Hourihane et al. (2023). In this work, we only inspect the comparison to WG11 in Fig. 17.
The median difference and standard deviation are given for each element. In general, the agreement is very good across the elements, with a spread on the order of typical uncertainties in abundance measurements. With a subset of the cross-match S1 shows an issue, though the bulk of the cross-match are in reasonable agreement. The error bars per CNAME are also large indicating greater uncertainty in the measurement of this element.

## 8. Conclusions

The homogenisation of the WG10 results across four SETUPs with analyses from multiple nodes that covered, often sparsely, different ranges in stellar parameters and chemical abundances was a challenging process. The goal was to produce a robust and well-calibrated single star catalogue that could be homogenised with the rest of the survey results. This meant optimally combining the node results following the WG11 Bayesian inference method for the WG10 and WG11 stellar parameters as well as for the WG11 chemical abundances, while for the WG10 chemical abundance, a simple per analysis calibration to WG11 was carried out. Crucial to the robustness of the final WG10 catalogue is understanding the quality of the results. In particular, the S/N, NN, and errors are key to refining the sample for any scientific study.

The final stellar parameters as a Kiel diagram and metallicity distribution, with a simple cleaning of S/N≥25 and NN≥2, is shown in Fig. 18. The scatter is considerably reduced in the Kiel diagram with respect to the full sample. The shift of the RGB with metallicity is clearly discernible. The metallicity distribution shows a left-handed asymmetry indicative of the metal-poor contribution from the thick disk. Small peaks at -1.5 and -2.4 coincide with globular cluster samples.

The final WG10 chemical abundances are shown in Fig. 19 as [X/Fe] against [Fe/H]. The abundances are binned by the NN that contributed to each abundance. The greater the NN, the clearer the morphology of the distribution, illustrating how these quality measures can be used to interpret this complex and intriguing dataset.

**Acknowledgements.** Based on data products from observations made with ESO Telescopes at the La Silla Paranal Observatory under programme ID 188.B-3002. These data products have been processed by the Cambridge Astronomy Survey Unit (CASU) at the Institute of Astronomy, University of Cambridge (supported by UKRI-STFC grants: ST/N005805/1, ST/T003081/1 and ST/X001857/1), and by the FLAMES/UVES reduction team at INAF/Osservatorio Astrofisico di Arcetri. These data have been obtained from the *Gaia*-ESO Survey Data Archive, prepared and hosted by the Wide Field Astronomy Unit, Institute for Astronomy, University of Edinburgh, which is funded by the UK Science and Technology Facilities Council. This work was partly supported by the European Union FP7 programme through ERC grant number 320360 and by the Leverhulme Trust through grant RPG-2012-541. We acknowledge the support from INAF and Ministero dell' Istruzione, dell' Università e della Ricerca (MIUR) in the form of the grant "Premiale VLT 2012". The results presented here benefit from discussions held during the *Gaia*-ESO workshops and conferences supported by the ESF (European Science Foundation) through the GREAT Research Network Programme. D.M. acknowledges financial support from the Agencia Estatal de Investigación 10.13039/501100011033 of the Ministerio de Ciencia e Innovación and the ERDF "A way of making Europe" through project PID2019-109522GB-C51. S.V. gratefully acknowledges the support provided by Fondecyt reg. 1220264 and by the ANID BASAL projects ACE210002 and FB210003. S.M. thanks the COST Action CA18104: MW-Gaia. U.H. acknowledges support from the Swedish National Space Agency (SNSA/Rymdstyrelsen). E.J.A. acknowledges financial support from the State

Agency for Research of the Spanish MCIU through the "Center of Excellence Severo Ochoa" award to the Instituto de Astrofísica de Andalucía (CEX2021-001131-S). T.B. was funded by the project grant no. 2018-04857 from the Swedish Research Council. G.G. acknowledges support by the Collaborative Research Centre SFB 881 (projects A5, A10), Heidelberg University, of the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) and by the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme (grant agreement 949173). P.J. acknowledges support from Fondecyt Regular Ladder Number 1231057, Mille- nium Nucleus ERIS NCN2021_017, Centros ANID Iniciativa Milenio. J.I.G.H. acknowledges financial support from the Spanish Ministry of Science and Innovation (MICINN) project PID2020-117493GB-I00. E.M. acknowledges financial support through a "Margarita Salas" postdoctoral fellowship from Universidad Complutense de Madrid (CT18/22), funded by the Spanish Ministerio de Universidades with NextGeneration EU funds.

## References

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Blomme, R., Daflon, S., Gebran, M., et al. 2022, A&A, 661, A120

Bragliaglia, A., Alfaro, E. J., Flaccomio, E., et al. 2022, A&A, 659, A200

Bressan, A., Marigo, P., Girardi, L., et al. 2012, MNRAS, 427, 127

Buder, S., Asplund, M., Duong, L., et al. 2018, MNRAS, 478, 4513

Buder, S., Sharma, S., Kos, J., et al. 2021, MNRAS, 506, 150

de Laverny, P., Recio-Blanco, A., Worley, C. C., & Plez, B. 2012, A&A, 544, A126

Den Hartog, E. A., Lawler, J. E., Sneden, C., & Cowan, J. J. 2003, Astrophys. J. Suppl. Ser., 148, 543

Denwood, M. J. 2016, J. Stat. Softw., 71

Franciosini, E., Randich, S., de Laverny, P., et al. 2022, A&A, 668, A49

Frasca, A., Alcalá, J. M., Covino, E., et al. 2003, A&A, 405, 149

Frasca, A., Guillout, P., Marilli, E., et al. 2006, A&A, 454, 301

Fuhr, J. R., Martin, G. A., & Wiese, W. L. 1988, J. Phys. Chem. Ref. Data, 17

García, G., & Campos, J. 1988, J. Quant. Spec. Radiat. Transf., 39, 477

Garz, T. 1973, A&A, 26, 471

Gavel, A., Gruyters, P., Heiter, U., et al. 2019, A&A, 629, A74

Gilmore, G., Randich, S., Worley, C. C., et al. 2022, A&A, 666, A120

Grevesse, N., Asplund, M., & Sauval, A. J. 2007, Space Sci. Rev., 130, 105

Gustafsson, B., Edvardsson, B., Eriksson, K., et al. 2008, A&A, 486, 951

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Ivarsson, S., Litzén, U., & Wahlgren, G. M. 2001, Physica Scripta, 64, 455

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Kurucz, R. L. 2008, Robert L. Kurucz on-line database of observed and predicted atomic transitions, http://kurucz.harvard.edu/atoms/

Kurucz, R. L. 2009, Robert L. Kurucz on-line database of observed and predicted atomic transitions, http://kurucz.harvard.edu/atoms/

Kurucz, R. L. 2010, Robert L. Kurucz on-line database of observed and predicted atomic transitions, http://kurucz.harvard.edu/atoms/

Kurucz, R. L. 2011, Robert L. Kurucz on-line database of observed and predicted atomic transitions, http://kurucz.harvard.edu/atoms/

Kurucz, R. L. 2012, Robert L. Kurucz on-line database of observed and predicted atomic transitions, http://kurucz.harvard.edu/atoms/

Kurucz, R. L. 2013, Robert L. Kurucz on-line database of observed and predicted atomic transitions, http://kurucz.harvard.edu/atoms/

Kurucz, R. L., & Peytremann, E. 1975, SAO Special Rep., 362, 1

Lanzafame, A. C., Frasca, A., Damiani, F., et al. 2015, A&A, 576, A80
The median difference and standard deviation are given for each element. In general, the agreement is very good across the elements, with a spread on the order of typical uncertainties in abundance measurements. With a subset of the cross-match S1 shows an issue, though the bulk of the cross-match are in reasonable agreement. The error bars per CNAME are also large indicating greater uncertainty in the measurement of this element.

## 8. Conclusions

The homogenisation of the WG10 results across four SETUPs with analyses from multiple nodes that covered, often sparsely, different ranges in stellar parameters and chemical abundances was a challenging process. The goal was to produce a robust and well-calibrated single star catalogue that could be homogenised with the rest of the survey results. This meant optimally combining the node results following the WG11 Bayesian inference method for the WG10 and WG11 stellar parameters as well as for the WG11 chemical abundances, while for the WG10 chemical abundance, a simple per analysis calibration to WG11 was carried out. Crucial to the robustness of the final WG10 catalogue is understanding the quality of the results. In particular, the S/N, NN, and errors are key to refining the sample for any scientific study.

The final stellar parameters as a Kiel diagram and metallicity distribution, with a simple cleaning of S/N≥25 and NN≥2, is shown in Fig. 18. The scatter is considerably reduced in the Kiel diagram with respect to the full sample. The shift of the RGB with metallicity is clearly discernible. The metallicity distribution shows a left-handed asymmetry indicative of the metal-poor contribution from the thick disk. Small peaks at -1.5 and -2.4 coincide with globular cluster samples.

The final WG10 chemical abundances are shown in Fig. 19 as [X/Fe] against [Fe/H]. The abundances are binned by the NN that contributed to each abundance. The greater the NN, the clearer the morphology of the distribution, illustrating how these quality measures can be used to interpret this complex and intriguing dataset.

**Acknowledgements.** Based on data products from observations made with ESO Telescopes at the La Silla Paranal Observatory under programme ID 188.B-3002. These data products have been processed by the Cambridge Astronomy Survey Unit (CASU) at the Institute of Astronomy, University of Cambridge (supported by UKRI-STFC grants: ST/N005805/1, ST/T003081/1 and ST/X001857/1), and by the FLAMES/UVES reduction team at INAF/Osservatorio Astrofisico di Arcetri. These data have been obtained from the *Gaia*-ESO Survey Data Archive, prepared and hosted by the Wide Field Astronomy Unit, Institute for Astronomy, University of Edinburgh, which is funded by the UK Science and Technology Facilities Council. This work was partly supported by the European Union FP7 programme through ERC grant number 320360 and by the Leverhulme Trust through grant RPG-2012-541. We acknowledge the support from INAF and Ministero dell' Istruzione, dell' Università e della Ricerca (MIUR) in the form of the grant "Premiale VLT 2012". The results presented here benefit from discussions held during the *Gaia*-ESO workshops and conferences supported by the ESF (European Science Foundation) through the GREAT Research Network Programme. D.M. acknowledges financial support from the Agencia Estatal de Investigación 10.13039/501100011033 of the Ministerio de Ciencia e Innovación and the ERDF "A way of making Europe" through project PID2019-109522GB-C51. S.V. gratefully acknowledges the support provided by Fondecyt reg. 1220264 and by the ANID BASAL projects ACE210002 and FB210003. S.M. thanks the COST Action CA18104: MW-Gaia. U.H. acknowledges support from the Swedish National Space Agency (SNSA/Rymdstyrelsen). E.J.A. acknowledges financial support from the State

Agency for Research of the Spanish MCIU through the "Center of Excellence Severo Ochoa" award to the Instituto de Astrofísica de Andalucía (CEX2021-001131-S). T.B. was funded by the project grant no. 2018-04857 from the Swedish Research Council. G.G. acknowledges support by the Collaborative Research Centre SFB 881 (projects A5, A10), Heidelberg University, of the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) and by the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme (grant agreement 949173). P.J. acknowledges support from Fondecyt Regular Ladder Number 1231057, Mille- nium Nucleus ERIS NCN2021_017, Centros ANID Iniciativa Milenio. J.I.G.H. acknowledges financial support from the Spanish Ministry of Science and Innovation (MICINN) project PID2020-117493GB-I00. E.M. acknowledges financial support through a "Margarita Salas" postdoctoral fellowship from Universidad Complutense de Madrid (CT18/22), funded by the Spanish Ministerio de Universidades with NextGeneration EU funds.

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3 Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, ul. Bartycka 18, 00-716, Warsaw, Poland

4 INAF – Osservatorio Astrofisico di Arcetri, Largo E. Fermi, 5, 50125 Firenze, Italy

5 Observational Astrophysics, Division of Astronomy and Space Physics, Department of Physics and Astronomy, Uppsala University, Box 516, 75120 Uppsala, Sweden

6 ROB – Royal Observatory of Belgium, Ringlaan 3, 1180 Brussels, Belgium

7 Dipartimento di Fisica e Astronomia, Sezione Astrofisica, Università di Catania, via S. Sofia 78, 95123 Catania, Italy

8 School of Physics & Astronomy, Monash University, Wellington Road, Clayton 3800, Victoria, Australia

9 INAF – Osservatorio Astrofisico di Catania, Via S. Sofia 78, 95123 Catania, Italy

10 GEPI, Observatoire de Paris, Université PSL, CNRS, 5 Place Jules Janssen, 92190 Meudon, France

11 Laboratoire d'astrophysique de Bordeaux, Univ. Bordeaux, CNRS, B18N, allée Geoffroy Saint-Hilaire, 33615 Pessac, France

12 Departamento de Física de la Tierra y Astrofísica & IPARCOS-UCM (Instituto de Física de Partículas y del Cosmos de la UCM), Facultad de Ciencias Físicas, Universidad Complutense de Madrid, 28040 Madrid, Spain

13 Lund Observatory, Division of Astrophysics, Department of Physics, Lund University, Box 43, 22100 Lund, Sweden

14 Lund Observatory, Department of Geology, Department of Physics, Lund University, Box 43, 22100 Lund, Sweden

15 Institute of Theoretical Physics and Astronomy, Vilnius University, Sauletekio av. 3, 10257 Vilnius, Lithuania

16 Department of Astronomy, Stockholm University, AlbaNova University Center, 106 91 Stockholm, Sweden

17 Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany

18 Centro de Astrobiología, CSIC-INTA, Camino bajo del castillo s/n, 28692, Villanueva de la Canàda, Madrid, Spain

19 Instituto de Astrofísica de Canarias, Vía Láctea s/n, 38205 La Laguna, Tenerife, Spain

20 Departamento de Astronomía, Casilla 160-C, Universidad de Concepción, Concepción, Chile

21 Astronomical Observatory, Institute of Theoretical Physics and Astronomy, Vilnius University, Sauletekio av. 3, 10257 Vilnius, Lithuania

22 Institut d'Astronomie et d'Astrophysique, Université Libre de Bruxelles, CP 226, Boulevard du Triomphe, 1050 Bruxelles, Belgium

23 Astrophysics Group, Keele University, Keele, Staffordshire ST5 5BG, UK

24 Institute for Astronomy, Royal Observatory, University of Edinburgh, Blackford Hill, Edinburgh EH9 3HJ, UK

25 GEPI, Observatoire de Paris, PSL Research University, CNRS, Univ. Paris Diderot, Sorbonne Paris Cité, 61 avenue de l'Observatoire, 75014 Paris, France

26 Université de Picardie Jules Verne, 33 rue St Leu, 80080 Amiens, France

27 INAF – Osservatorio di Astrofisica e Scienza dello Spazio, via P. Gobetti 93/3, 40129 Bologna, Italy

28 Instituto de Astrofísica de Andalucía, CSIC, Glorieta de la Astronomía s/n, Granada 18008, Spain

29 Institute of Astrophysics, FORTH, Crete, Greece

30 INAF – Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, 35122 Padova, Italy

31 European Space Agency (ESA), European Space Research and Technology Centre (ESTEC), Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands

32 INAF – Osservatorio Astronomico di Roma, Via Frascati 33, 00040 Monte Porzio Catone (Roma), Italy

33 Núcleo Milenio ERIS & Instituto de Estudios Astrofísicos, Universidad Diego Portales, Ejército 441, Santiago, Chile

34 Hamburger Sternwarte, Gojenbergsweg 112, 21029 Hamburg, Germany

<footnote n="1">¹ Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
e-mail: ccworley@ast.cam.ac.uk;
clare.worley@canterbury.ac.nz</footnote>

<footnote n="2">² School of Physical and Chemical Sciences – Te Kura Matū, University of Canterbury, Private Bag 4800, Christchurch 8140, New Zealand</footnote>
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3 Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, ul. Bartycka 18, 00-716, Warsaw, Poland

4 INAF – Osservatorio Astrofisico di Arcetri, Largo E. Fermi, 5, 50125 Firenze, Italy

5 Observational Astrophysics, Division of Astronomy and Space Physics, Department of Physics and Astronomy, Uppsala University, Box 516, 75120 Uppsala, Sweden

6 ROB – Royal Observatory of Belgium, Ringlaan 3, 1180 Brussels, Belgium

7 Dipartimento di Fisica e Astronomia, Sezione Astrofisica, Università di Catania, via S. Sofia 78, 95123 Catania, Italy

8 School of Physics & Astronomy, Monash University, Wellington Road, Clayton 3800, Victoria, Australia

9 INAF – Osservatorio Astrofisico di Catania, Via S. Sofia 78, 95123 Catania, Italy

10 GEPI, Observatoire de Paris, Université PSL, CNRS, 5 Place Jules Janssen, 92190 Meudon, France

11 Laboratoire d'astrophysique de Bordeaux, Univ. Bordeaux, CNRS, B18N, allée Geoffroy Saint-Hilaire, 33615 Pessac, France

12 Departamento de Física de la Tierra y Astrofísica & IPARCOS-UCM (Instituto de Física de Partículas y del Cosmos de la UCM), Facultad de Ciencias Físicas, Universidad Complutense de Madrid, 28040 Madrid, Spain

13 Lund Observatory, Division of Astrophysics, Department of Physics, Lund University, Box 43, 22100 Lund, Sweden

14 Lund Observatory, Department of Geology, Department of Physics, Lund University, Box 43, 22100 Lund, Sweden

15 Institute of Theoretical Physics and Astronomy, Vilnius University, Sauletekio av. 3, 10257 Vilnius, Lithuania

16 Department of Astronomy, Stockholm University, AlbaNova University Center, 106 91 Stockholm, Sweden

17 Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany

18 Centro de Astrobiología, CSIC-INTA, Camino bajo del castillo s/n, 28692, Villanueva de la Canàda, Madrid, Spain

19 Instituto de Astrofísica de Canarias, Vía Láctea s/n, 38205 La Laguna, Tenerife, Spain

20 Departamento de Astronomía, Casilla 160-C, Universidad de Concepción, Concepción, Chile

21 Astronomical Observatory, Institute of Theoretical Physics and Astronomy, Vilnius University, Sauletekio av. 3, 10257 Vilnius, Lithuania

22 Institut d'Astronomie et d'Astrophysique, Université Libre de Bruxelles, CP 226, Boulevard du Triomphe, 1050 Bruxelles, Belgium

23 Astrophysics Group, Keele University, Keele, Staffordshire ST5 5BG, UK

24 Institute for Astronomy, Royal Observatory, University of Edinburgh, Blackford Hill, Edinburgh EH9 3HJ, UK

25 GEPI, Observatoire de Paris, PSL Research University, CNRS, Univ. Paris Diderot, Sorbonne Paris Cité, 61 avenue de l'Observatoire, 75014 Paris, France

26 Université de Picardie Jules Verne, 33 rue St Leu, 80080 Amiens, France

27 INAF – Osservatorio di Astrofisica e Scienza dello Spazio, via P. Gobetti 93/3, 40129 Bologna, Italy

28 Instituto de Astrofísica de Andalucía, CSIC, Glorieta de la Astronomía s/n, Granada 18008, Spain

29 Institute of Astrophysics, FORTH, Crete, Greece

30 INAF – Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, 35122 Padova, Italy

31 European Space Agency (ESA), European Space Research and Technology Centre (ESTEC), Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands

32 INAF – Osservatorio Astronomico di Roma, Via Frascati 33, 00040 Monte Porzio Catone (Roma), Italy

33 Núcleo Milenio ERIS & Instituto de Estudios Astrofísicos, Universidad Diego Portales, Ejército 441, Santiago, Chile

34 Hamburger Sternwarte, Gojenbergsweg 112, 21029 Hamburg, Germany

<footnote n="1">¹ Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
e-mail: ccworley@ast.cam.ac.uk;
clare.worley@canterbury.ac.nz</footnote>

<footnote n="2">² School of Physical and Chemical Sciences – Te Kura Matū, University of Canterbury, Private Bag 4800, Christchurch 8140, New Zealand</footnote>
## Appendix A: Working Group 10 spectral line information

<table><caption>Table A.1. Spectral lines used by WG10 Nodes.</caption><thead><tr><th>Species</th><th>Wavelength (Å)</th></tr></thead><tbody><tr><td>Al I</td><td>5557.06, 6696.02, 6698.67, 8772.87, 8773.90</td></tr><tr><td>Ba II</td><td>6496.90</td></tr><tr><td>C I</td><td>5380.33, 6587.61</td></tr><tr><td>Ca I</td><td>5260.39, 5261.70, 5349.46, 5581.96, 5590.11, 6455.60, 6471.66, 6493.78, 6499.65</td></tr><tr><td>Ca II</td><td>8498.02, 8542.09, 8662.14, 8912.07</td></tr><tr><td>Ce II</td><td>5187.46, 5274.23, 5330.56</td></tr><tr><td>Co I</td><td>5176.08, 5212.69, 5280.63, 5301.04, 5331.45, 5352.04, 5352.07, 5530.73, 5530.78, 5590.66, 5590.74, 6454.99, 6632.44, 6771.02, 6771.03</td></tr><tr><td>Cr I</td><td>5200.17, 5206.02, 5238.96, 5241.46, 5247.56, 5272.00, 5287.18, 5296.69, 5300.75, 5304.18, 5312.86, 5318.77, 5345.80, 5348.31, 5409.78</td></tr><tr><td>Cr II</td><td>5246.77</td></tr><tr><td>Cu I</td><td>5218.20, 5220.07</td></tr><tr><td>Dy II</td><td>5169.69</td></tr><tr><td>Eu II</td><td>6645.06, 6645.10</td></tr><tr><td>Fe I</td><td>5159.06, 5194.94, 5197.94, 5198.71, 5215.18, 5216.27, 5217.39, 5223.18, 5225.53, 5228.38, 5232.94, 5236.20, 5242.49, 5243.78, 5247.05, 5250.21, 5250.65, 5253.02, 5253.46, 5262.88, 5263.31, 5269.54, 5273.16, 5279.65, 5285.13, 5288.52, 5293.96, 5294.55, 5295.31, 5300.40, 5302.30, 5320.04, 5321.11, 5322.04, 5324.18, 5339.93, 5364.87, 5367.47, 5373.71, 5379.57, 5383.37, 5386.33, 5389.48, 5393.17, 5397.13, 5398.28, 5405.77, 5410.91, 5415.20, 5417.03, 5424.07, 5429.70, 5434.52, 5441.34, 5445.04, 5455.61, 5466.40, 5473.90, 5491.83, 5501.46, 5506.78, 5522.45, 5525.54, 5536.58, 5538.52, 5539.28, 5543.94, 5546.51, 5560.21, 5569.62, 5572.84, 5576.09, 5586.76, 6475.62, 6481.87, 6494.98, 6495.74, 6496.47, 6498.94, 6518.37, 6533.93, 6546.24, 6569.21, 6574.23, 6581.21, 6592.91, 6593.87, 6597.56, 6608.02, 6609.11, 6627.54, 6633.41, 6633.75, 6634.11, 6648.08, 6699.14, 6703.57, 6705.10, 6713.05, 6713.74, 6725.36, 6733.15, 6739.52, 6750.15, 6752.71, 6786.86, 6793.26, 8514.07, 8515.11, 8571.80, 8582.26, 8598.83, 8611.80, 8621.60, 8688.62, 8699.45, 8784.44, 8824.22, 8846.74</td></tr><tr><td>Fe II</td><td>5169.03, 5197.57, 5234.62, 5256.93, 5264.80, 5284.10, 5316.61, 5316.78, 5325.55, 5425.25, 6442.96, 6456.38, 6516.08</td></tr><tr><td>La II</td><td>5303.53</td></tr><tr><td>Li I</td><td>6707.76, 6707.91</td></tr><tr><td>Mg I</td><td>5167.32, 5172.68, 5183.60, 5528.40, 8717.83, 8736.02, 8806.76</td></tr><tr><td>Mn I</td><td>5394.62, 5394.67, 5420.35, 5420.42, 5432.50, 6440.93</td></tr><tr><td>Mo I</td><td>5570.44</td></tr><tr><td>Nd II</td><td>5276.87, 5311.45, 5319.81, 5431.52, 6637.19</td></tr><tr><td>Ni I</td><td>5157.98, 5424.65, 5435.86, 5578.72, 5587.86, 6482.80, 6532.87, 6586.31, 6643.63, 6767.77</td></tr><tr><td>Pr II</td><td>5259.73, 5322.77</td></tr><tr><td>S I</td><td>6743.48, 6743.54, 6743.58, 6748.57, 6748.58, 6748.79, 6757.15</td></tr><tr><td>Sc II</td><td>5526.79, 6604.60</td></tr><tr><td>Si I</td><td>6721.85, 6741.63, 8892.72</td></tr><tr><td>Sr I</td><td>6546.78, 6791.02</td></tr><tr><td>Ti I</td><td>5145.46, 5147.48, 5152.18, 5210.38, 5219.70, 5223.62, 5224.30, 5230.97, 5282.38, 5295.78, 5300.01, 5338.31, 5426.25, 5471.19, 5490.15, 5514.53, 6497.68, 6554.22, 6556.06, 6599.10, 8682.98, 8734.71</td></tr><tr><td>Ti II</td><td>5185.90, 5211.53, 5336.79, 5381.02, 5418.77</td></tr><tr><td>V I</td><td>5604.90, 6531.42</td></tr><tr><td>Y II</td><td>5200.41, 5205.72, 5289.81, 5402.77, 5544.61, 6795.41</td></tr><tr><td>Zr I</td><td>5385.14, 6445.74</td></tr></tbody></table>

Notes. Species and wavelength of spectral lines for which abundances were measured by the WG10 nodes for the WG10 setups. See the Gaia-ESO linelist (Heiter et al. 2021) for the complete information per line.
Appendix A: Working Group 10 spectral line information

<table><caption>Table A.1. Spectral lines used by WG10 Nodes.</caption><thead><tr><th>Species</th><th>Wavelength (Å)</th></tr></thead><tbody><tr><td>Al I</td><td>5557.06, 6696.02, 6698.67, 8772.87, 8773.90</td></tr><tr><td>Ba II</td><td>6496.90</td></tr><tr><td>C I</td><td>5380.33, 6587.61</td></tr><tr><td>Ca I</td><td>5260.39, 5261.70, 5349.46, 5581.96, 5590.11, 6455.60, 6471.66, 6493.78, 6499.65</td></tr><tr><td>Ca II</td><td>8498.02, 8542.09, 8662.14, 8912.07</td></tr><tr><td>Ce II</td><td>5187.46, 5274.23, 5330.56</td></tr><tr><td>Co I</td><td>5176.08, 5212.69, 5280.63, 5301.04, 5331.45, 5352.04, 5352.07, 5530.73, 5530.78, 5590.66, 5590.74, 6454.99, 6632.44, 6771.02, 6771.03</td></tr><tr><td>Cr I</td><td>5200.17, 5206.02, 5238.96, 5241.46, 5247.56, 5272.00, 5287.18, 5296.69, 5300.75, 5304.18, 5312.86, 5318.77, 5345.80, 5348.31, 5409.78</td></tr><tr><td>Cr II</td><td>5246.77</td></tr><tr><td>Cu I</td><td>5218.20, 5220.07</td></tr><tr><td>Dy II</td><td>5169.69</td></tr><tr><td>Eu II</td><td>6645.06, 6645.10</td></tr><tr><td>Fe I</td><td>5159.06, 5194.94, 5197.94, 5198.71, 5215.18, 5216.27, 5217.39, 5223.18, 5225.53, 5228.38, 5232.94, 5236.20, 5242.49, 5243.78, 5247.05, 5250.21, 5250.65, 5253.02, 5253.46, 5262.88, 5263.31, 5269.54, 5273.16, 5279.65, 5285.13, 5288.52, 5293.96, 5294.55, 5295.31, 5300.40, 5302.30, 5320.04, 5321.11, 5322.04, 5324.18, 5339.93, 5364.87, 5367.47, 5373.71, 5379.57, 5383.37, 5386.33, 5389.48, 5393.17, 5397.13, 5398.28, 5405.77, 5410.91, 5415.20, 5417.03, 5424.07, 5429.70, 5434.52, 5441.34, 5445.04, 5455.61, 5466.40, 5473.90, 5491.83, 5501.46, 5506.78, 5522.45, 5525.54, 5536.58, 5538.52, 5539.28, 5543.94, 5546.51, 5560.21, 5569.62, 5572.84, 5576.09, 5586.76, 6475.62, 6481.87, 6494.98, 6495.74, 6496.47, 6498.94, 6518.37, 6533.93, 6546.24, 6569.21, 6574.23, 6581.21, 6592.91, 6593.87, 6597.56, 6608.02, 6609.11, 6627.54, 6633.41, 6633.75, 6634.11, 6648.08, 6699.14, 6703.57, 6705.10, 6713.05, 6713.74, 6725.36, 6733.15, 6739.52, 6750.15, 6752.71, 6786.86, 6793.26, 8514.07, 8515.11, 8571.80, 8582.26, 8598.83, 8611.80, 8621.60, 8688.62, 8699.45, 8784.44, 8824.22, 8846.74</td></tr><tr><td>Fe II</td><td>5169.03, 5197.57, 5234.62, 5256.93, 5264.80, 5284.10, 5316.61, 5316.78, 5325.55, 5425.25, 6442.96, 6456.38, 6516.08</td></tr><tr><td>La II</td><td>5303.53</td></tr><tr><td>Li I</td><td>6707.76, 6707.91</td></tr><tr><td>Mg I</td><td>5167.32, 5172.68, 5183.60, 5528.40, 8717.83, 8736.02, 8806.76</td></tr><tr><td>Mn I</td><td>5394.62, 5394.67, 5420.35, 5420.42, 5432.50, 6440.93</td></tr><tr><td>Mo I</td><td>5570.44</td></tr><tr><td>Nd II</td><td>5276.87, 5311.45, 5319.81, 5431.52, 6637.19</td></tr><tr><td>Ni I</td><td>5157.98, 5424.65, 5435.86, 5578.72, 5587.86, 6482.80, 6532.87, 6586.31, 6643.63, 6767.77</td></tr><tr><td>Pr II</td><td>5259.73, 5322.77</td></tr><tr><td>S I</td><td>6743.48, 6743.54, 6743.58, 6748.57, 6748.58, 6748.79, 6757.15</td></tr><tr><td>Sc II</td><td>5526.79, 6604.60</td></tr><tr><td>Si I</td><td>6721.85, 6741.63, 8892.72</td></tr><tr><td>Sr I</td><td>6546.78, 6791.02</td></tr><tr><td>Ti I</td><td>5145.46, 5147.48, 5152.18, 5210.38, 5219.70, 5223.62, 5224.30, 5230.97, 5282.38, 5295.78, 5300.01, 5338.31, 5426.25, 5471.19, 5490.15, 5514.53, 6497.68, 6554.22, 6556.06, 6599.10, 8682.98, 8734.71</td></tr><tr><td>Ti II</td><td>5185.90, 5211.53, 5336.79, 5381.02, 5418.77</td></tr><tr><td>V I</td><td>5604.90, 6531.42</td></tr><tr><td>Y II</td><td>5200.41, 5205.72, 5289.81, 5402.77, 5544.61, 6795.41</td></tr><tr><td>Zr I</td><td>5385.14, 6445.74</td></tr></tbody></table>

Notes. Species and wavelength of spectral lines for which abundances were measured by the WG10 nodes for the WG10 setups. See the Gaia-ESO linelist (Heiter et al. 2021) for the complete information per line.
Appendix B: Working Group 10 element abundance corrections

<table><caption>Table B.1. Coefficients of WG10 bias corrections.</caption><thead><tr><th>SETUP</th><th>NODE</th><th>ELEMENT</th><th>IP</th><th>a0</th><th>a1</th><th>a2</th><th>a3</th><th>min(IP)</th><th>max(IP)</th><th>MedianA</th><th>σA</th><th>Calibration</th></tr></thead><tbody><tr><td>HRT0</td><td>CAUP</td><td>CA1</td><td>FEH_D</td><td>-0.0128635771</td><td>-0.0853183007</td><td>-</td><td>-</td><td>-2.52</td><td>0.32</td><td>0.0000</td><td>0.1878</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>CAUP</td><td>CA1</td><td>FEH_G</td><td>0.0671735328</td><td>0.0720870430</td><td>-</td><td>-</td><td>-2.00</td><td>0.21</td><td>-0.0100</td><td>0.1762</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>CAUP</td><td>CO1</td><td>FEH_D</td><td>-0.1904706240</td><td>0.0279439500</td><td>-</td><td>-</td><td>-0.30</td><td>0.41</td><td>-0.1800</td><td>0.0902</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>CAUP</td><td>CO1</td><td>FEH_G</td><td>-0.0299998950</td><td>-</td><td>-</td><td>-</td><td>-1.21</td><td>0.21</td><td>-0.0300</td><td>0.0824</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>CAUP</td><td>CR1</td><td>LOGG_D</td><td>-5.6450875166</td><td>2.8491813136</td><td>-0.3506320046</td><td>-</td><td>3.53</td><td>4.59</td><td>0.0800</td><td>0.1470</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>CAUP</td><td>CR1</td><td>FEH_G</td><td>0.0624965243</td><td>-0.0223026185</td><td>-0.0403518382</td><td>-</td><td>-2.62</td><td>0.21</td><td>0.0200</td><td>0.3286</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>CAUP</td><td>FE1</td><td>LOGG_D</td><td>-0.0379078330</td><td>-0.0468408820</td><td>0.0117258380</td><td>-</td><td>0.95</td><td>4.68</td><td>-0.0600</td><td>0.1338</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>CAUP</td><td>FE1</td><td>FEH_G</td><td>-0.0388349210</td><td>0.02757011220</td><td>-0.0078109530</td><td>-</td><td>-2.52</td><td>0.04</td><td>-0.0500</td><td>0.1593</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>CAUP</td><td>MN1</td><td>FEH_D</td><td>-0.2178134436</td><td>-0.1944580752</td><td>-</td><td>-</td><td>-0.25</td><td>0.45</td><td>-0.2200</td><td>0.1458</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>CAUP</td><td>MN1</td><td>FEH_G</td><td>-0.3584931025</td><td>-0.0358944088</td><td>-</td><td>-</td><td>-1.54</td><td>0.21</td><td>-0.3100</td><td>0.1742</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>CAUP</td><td>NI1</td><td>FEH_D</td><td>-0.0322487332</td><td>-0.2028706638</td><td>-</td><td>-</td><td>-0.70</td><td>0.45</td><td>0.0100</td><td>0.1130</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>CAUP</td><td>NI1</td><td>FEH_G</td><td>-0.0539072155</td><td>-0.0685051063</td><td>-</td><td>-</td><td>-1.54</td><td>0.21</td><td>0.0200</td><td>0.1747</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>CAUP</td><td>SC2</td><td>FEH_D</td><td>-0.141620289</td><td>-0.1317874827</td><td>-</td><td>-</td><td>-1.10</td><td>0.45</td><td>-0.1300</td><td>0.1385</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>CAUP</td><td>SC2</td><td>FEH_G</td><td>-0.3906970169</td><td>-0.5386362834</td><td>-0.1670547663</td><td>-</td><td>-1.10</td><td>0.21</td><td>-0.0400</td><td>0.1691</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>CAUP</td><td>TI2</td><td>FEH_D</td><td>-0.1060732326</td><td>-0.0850312307</td><td>-</td><td>-</td><td>-2.52</td><td>0.45</td><td>-0.1100</td><td>0.1078</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>CAUP</td><td>TI2</td><td>FEH_G</td><td>-0.317366324</td><td>-0.3105625844</td><td>-0.0567801729</td><td>-</td><td>-2.62</td><td>0.21</td><td>-0.0800</td><td>0.2249</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>C1</td><td>FEH_D</td><td>0.0732768207</td><td>-0.0491589552</td><td>-</td><td>-</td><td>-0.70</td><td>0.45</td><td>-0.0500</td><td>0.1135</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>C1</td><td>OFFSET_G</td><td>0.2500</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>0.2500</td><td>0.0683</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>CO1</td><td>OFFSET_D</td><td>-0.0500</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-0.0500</td><td>0.1646</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>CO1</td><td>FEH_G</td><td>-0.0313088310</td><td>0.0788521830</td><td>0.1184216920</td><td>-</td><td>-</td><td>-1.26</td><td>0.04</td><td>0.0200</td><td>0.1091</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>CR1</td><td>TEFF_D</td><td>-16.7383167700</td><td>0.0061316870</td><td>-0.0000005546</td><td>-</td><td>4842</td><td>6483</td><td>0.1100</td><td>0.1228</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>CR1</td><td>TEFF_G</td><td>6.7606788150</td><td>-0.0022318690</td><td>0.0000001747</td><td>-</td><td>4423</td><td>6720</td><td>0.0300</td><td>0.2739</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>FE1</td><td>FEH_G</td><td>0.0976131640</td><td>0.0838707160</td><td>0.0123411550</td><td>-</td><td>-2.52</td><td>0.37</td><td>0.0700</td><td>0.2463</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>FE1</td><td>LOGG_D</td><td>4.3500420690</td><td>-2.2274475100</td><td>0.2789431000</td><td>-</td><td>3.45</td><td>4.68</td><td>-0.0700</td><td>0.1282</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>MG1</td><td>FEH</td><td>0.0464074730</td><td>-0.0687944546</td><td>-</td><td>-</td><td>-1.10</td><td>0.45</td><td>0.0600</td><td>0.1221</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>MN1</td><td>FEH</td><td>-0.0721551932</td><td>-0.2434403206</td><td>-0.2944977537</td><td>-</td><td>-1.10</td><td>0.30</td><td>-0.1200</td><td>0.2009</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>MO1</td><td>FEH</td><td>0.4932369290</td><td>1.3317375180</td><td>-0.6803415420</td><td>-3.55216122</td><td>-0.49</td><td>0.35</td><td>0.5000</td><td>3.8600</td><td>WG11-full</td></tr><tr><td>HRT0</td><td>Lumba</td><td>ND2</td><td>OFFSET_D</td><td>0.7200</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>0.7200</td><td>0.1259</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>ND2</td><td>FEH_G</td><td>0.5507316480</td><td>0.6873607020</td><td>0.2871853550</td><td>-</td><td>-</td><td>-1.23</td><td>0.04</td><td>0.0200</td><td>0.1836</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>NI1</td><td>FEH_D</td><td>0.113103971</td><td>0.0412906286</td><td>-</td><td>-</td><td>-0.40</td><td>0.45</td><td>0.1000</td><td>0.1028</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>NI1</td><td>OFFSET_G</td><td>0.1800</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>0.1800</td><td>0.1969</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>SC2</td><td>OFFSET_D</td><td>-0.1100</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-0.1100</td><td>0.1490</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>SC2</td><td>OFFSET_G</td><td>0.0700</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>0.0700</td><td>0.1842</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>V1</td><td>OFFSET_D</td><td>-0.0800</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-0.0800</td><td>0.0283</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>V1</td><td>OFFSET_G</td><td>-0.0400</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-0.0400</td><td>0.0752</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>Y2</td><td>OFFSET_D</td><td>-0.2300</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-0.2300</td><td>0.1245</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>Y2</td><td>OFFSET_G</td><td>-0.0900</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-0.0900</td><td>0.1608</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>ZR1</td><td>FEH</td><td>0.1523604990</td><td>0.5486256480</td><td>1.1509851220</td><td>0.65947002</td><td>-</td><td>-1.25</td><td>0.37</td><td>0.1300</td><td>4.4100</td><td>WG11-full</td></tr><tr><td>HRT0</td><td>Lumba</td><td>AL1</td><td>FEH_D</td><td>0.0598238978</td><td>0.0004466455</td><td>-</td><td>-</td><td>-0.70</td><td>0.45</td><td>-0.0800</td><td>0.0455</td><td>0.1454</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>AL1</td><td>FEH_G</td><td>0.1159365538</td><td>-0.0363255123</td><td>-</td><td>-</td><td>-1.50</td><td>0.21</td><td>0.1800</td><td>0.1879</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>CA1</td><td>FEH_D</td><td>0.1303592641</td><td>0.0529698156</td><td>-</td><td>-</td><td>-0.70</td><td>0.45</td><td>0.1400</td><td>0.1557</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>CA1</td><td>OFFSET_G</td><td>0.0400</td><td>-</td><td>-</td><td>-</td><td>-1.10</td><td>0.21</td><td>0.0400</td><td>0.1886</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>CO1</td><td>FEH_D</td><td>0.1415773330</td><td>0.0838384140</td><td>-0.0796160610</td><td>-</td><td>-0.71</td><td>0.41</td><td>0.1200</td><td>0.1454</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>CO1</td><td>FEH_G</td><td>0.2384163850</td><td>0.2857059710</td><td>0.1121185940</td><td>-</td><td>-1.26</td><td>0.37</td><td>0.0600</td><td>0.2132</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>CR1</td><td>LOGG_D</td><td>3.141860370</td><td>-1.5389358300</td><td>0.1933153520</td><td>-</td><td>3.45</td><td>4.68</td><td>0.0900</td><td>0.1543</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>CR1</td><td>LOGG_G</td><td>0.3495480500</td><td>-0.4913832760</td><td>0.1403916450</td><td>-</td><td>0.95</td><td>3.39</td><td>-0.0200</td><td>0.2645</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>FE1</td><td>LOGG_D</td><td>2.6557655300</td><td>-1.3217719570</td><td>0.1695725040</td><td>-</td><td>3.45</td><td>4.68</td><td>0.1000</td><td>0.1555</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>FE1</td><td>FEH_G</td><td>0.2328755010</td><td>0.1948311820</td><td>0.0523083140</td><td>-</td><td>-2.52</td><td>0.37</td><td>0.0900</td><td>0.2349</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>FE2</td><td>LOGG</td><td>0.6344379240</td><td>-0.2852883300</td><td>0.0442309150</td><td>-</td><td>0.95</td><td>4.68</td><td>-0.0200</td><td>0.2018</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>MG1</td><td>OFFSET_D</td><td>0.1600</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-0.1600</td><td>0.1779</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>MG1</td><td>FEH_G</td><td>-0.0406796642</td><td>-0.3352504432</td><td>-</td><td>-</td><td>-1.10</td><td>0.21</td><td>0.1600</td><td>0.2601</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>MN1</td><td>TEFF_D</td><td>-1.4101857502</td><td>0.0004340610</td><td>-0.0000000316</td><td>-</td><td>4256</td><td>6756</td><td>0.0100</td><td>0.1615</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>MN1</td><td>FEH_G</td><td>0.0285548670</td><td>0.1218215121</td><td>-</td><td>-</td><td>-1.54</td><td>0.21</td><td>-0.0900</td><td>0.1970</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>NI1</td><td>LOGG_D</td><td>6.1505396041</td><td>-3.1638494044</td><td>0.4061924846</td><td>-</td><td>3.53</td><td>4.51</td><td>0.0500</td><td>0.1508</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>NI1</td><td>TEFF_G</td><td>9.0197287067</td><td>-0.0035566944</td><td>0.00000003496</td><td>-</td><td>-1.26</td><td>0.37</td><td>0.0000</td><td>0.2335</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>TI1</td><td>FEH_D</td><td>0.1215496359</td><td>0.0156832702</td><td>-</td><td>-</td><td>-0.70</td><td>0.45</td><td>0.1600</td><td>0.2127</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>TI1</td><td>FEH_G</td><td>-0.207111023</td><td>-0.210711023</td><td>-</td><td>-</td><td>-0.70</td><td>0.00</td><td>0.2000</td><td>0.2336</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>TI2</td><td>FEH_G</td><td>0.3898855087</td><td>-</td><td>-</td><td>-</td><td>-2.62</td><td>0.21</td><td>0.3300</td><td>0.2773</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>TI2</td><td>FEH_D</td><td>0.1096975581</td><td>-0.0688373436</td><td>-0.0399396966</td><td>-</td><td>-2.03</td><td>0.45</td><td>0.1100</td><td>0.2071</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>Y2</td><td>OFFSET_D</td><td>-0.0200</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-0.0200</td><td>0.2140</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>Y2</td><td>OFFSET_G</td><td>0.0700</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-0.70</td><td>0.1200</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>CAUP</td><td>CA1</td><td>FEH_D</td><td>-0.0987282970</td><td>-0.0744936740</td><td>0.0912179140</td><td>-</td><td>-1.27</td><td>0.20</td><td>0.0700</td><td>0.2044</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>CAUP</td><td>CA1</td><td>FEH_G</td><td>-0.0558260260</td><td>-0.0515666940</td><td>-0.0056638010</td><td>-</td><td>-2.54</td><td>0.32</td><td>-0.0500</td><td>0.1928</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>CAUP</td><td>FE1</td><td>TEFF_D</td><td>1.5395375310</td><td>-0.0005183000</td><td>0.0000000444</td><td>-</td><td>4092</td><td>629</td><td>0.0400</td><td>0.1498</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>CAUP</td><td>FE1</td><td>TEFF_G</td><td>6.0155818810</td><td>-0.0025553130</td><td>0.00000002721</td><td>-</td><td>4171</td><td>5132</td><td>0.0400</td><td>0.1189</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>CAUP</td><td>NI1</td><td>TEFF_G</td><td>0.9724628770</td><td>0.0003342880</td><td>0.0000000277</td><td>-</td><td>4092</td><td>5132</td><td>0.0200</td><td>0.1552</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>CAUP</td><td>NI1</td><td>TEFF_G</td><td>9.5562424000</td><td>-0.0041799340</td><td>0.0000004513</td><td>-</td><td>4171</td><td>5132</td><td>-0.0800</td><td>0.1454</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>CAUP</td><td>SC2</td><td>FEH_D</td><td>0.01003669214</td><td>-0.1982793021</td><td>-</td><td>-</td><td>-1.00</td><td>0.00</td><td>-0.0900</td><td>0.1188</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>CAUP</td><td>SC2</td><td>FEH_G</td><td>-0.1855341097</td><td>-0.1870818927</td><td>-</td><td>-</td><td>-1.66</td><td>0.33</td><td>-0.1300</td><td>0.1105</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>CAUP</td><td>SI1</td><td>FEH_D</td><td>0.0506171736</td><td>0.0450048868</td><td>-</td><td>-</td><td>-0.86</td><td>0.49</td><td>0.0500</td><td>0.1275</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>CAUP</td><td>SI1</td><td>FEH_G</td><td>0.0823885530</td><td>0.2563482820</td><td>0.3457082370</td><td>-</td><td>-0.86</td><td>0.29</td><td>0.0600</td><td>0.1468</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>AL1</td><td>TEFF_D</td><td>-0.9569700663</td><td>0.0005238327</td><td>-0.0000000558</td><td>-</td><td>5003</td><td>6710</td><td>0.2060</td><td>0.2588</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>AL1</td><td>FEH_G</td><td>0.3162735083</td><td>0.2239841044</td><td>0.0792369502</td><td>-</td><td>-1.66</td><td>0.33</td><td>0.2550</td><td>0.1659</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>BA2</td><td>FEH_D</td><td>0.0985018910</td><td>-0.7698388700</td><td>-0.5755655770</td><td>-0.13481981</td><td>-2.09</td><td>0.32</td><td>0.1310</td><td>2.9850</td><td>WG11-full</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>BA2</td><td>FEH_G</td><td>-0.4055081900</td><td>0.0141792960</td><td>1.4568006990</td><td>0.66517806</td><td>-2.54</td><td>0.17</td><td>0.0560</td><td>0.26590</td><td>WG11-full</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>C1</td><td>OFFSET_D</td><td>0.0800</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-0.0800</td><td>0.1779</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>CA1</td><td>FEH_G</td><td>0.0846544789</td><td>-0.2307559980</td><td>-</td><td>-</td><td>-0.42</td><td>0.33</td><td>0.1400</td><td>0.1920</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>CA1</td><td>OFFSET_D</td><td>0.1740</td><td>-</td><td>-</td><td>-</td><td>-0.56</td><td>0.49</td><td>0.1740</td><td>0.1957</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>CA1</td><td>FEH_G</td><td>0.1069150534</td><td>0.2156591825</td><td>0.1333802684</td><td>-</td><td>-1.66</td><td>0.29</td><td>0.0640</td><td>0.1319</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>CA1</td><td>FEH_D</td><td>0.1945363800</td><td>-0.1662533510</td><td>0.3524026810</td><td>-</td><td>-2.20</td><td>0.36</td><td>0.1980</td><td>0.3100</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>CO1</td><td>FEH_G</td><td>0.2644097580</td><td>-0.0484794770</td><td>-0.1019780170</td><td>-</td><td>-1.66</td><td>0.29</td><td>0.2180</td><td>0.2778</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EU2</td><td>EU2</td><td>OFFSET_D</td><td>0.0590</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>0.0590</td><td>0.1505</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>EU2</td><td>FEH_G</td><td>0.1269190636</td><td>0.1666165730</td><td>-</td><td>-</td><td>-1.58</td><td>0.33</td><td>0.0250</td><td>0.1917</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>FE1</td><td>FEH_D</td><td>0.0462124040</td><td>-0.2231415800</td><td>0.4096522430</td><td>-</td><td>-0.75</td><td>0.36</td><td>0.0790</td><td>0.3726</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>FE1</td><td>FEH_G</td><td>0.0987415140</td><td>0.2070314350</td><td>0.1384381260</td><td>-</td><td>-2.20</td><td>0.36</td><td>0.0810</td><td>0.2919</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>FE1</td><td>FEH_D</td><td>0.2666048930</td><td>0.0828850200</td><td>-</td><td>-</td><td>-1.20</td><td>0.36</td><td>0.2730</td><td>0.3504</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>FE2</td><td>FEH_G</td><td>0.3398705230</td><td>0.1513853770</td><td>-</td><td>-</td><td>-1.66</td><td>0.29</td><td>0.2750</td><td>0.2321</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>SRI</td><td>OFFSET</td><td>1.6330</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-1.6330</td><td>1.6330</td><td>Scaled Solar</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>TII</td><td>TEFF_D</td><td>17.1293465052</td><td>-0.0064595794</td><td>0.0000006138</td><td>-</td><td>5003</td><td>6300</td><td>0.3030</td><td>0.4986</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>TII</td><td>TEFF_G</td><td>-9.9478595742</td><td>0.0044616249</td><td>-0.0000004934</td><td>-</td><td>4269</td><td>5100</td><td>0.1020</td><td>0.1317</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>V1</td><td>FEH_D</td><td>0.0867662461</td><td>-0.3446519198</td><td>-</td><td>-</td><td>-0.51</td><td>0.49</td><td>0.1100</td><td>0.4483</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>V1</td><td>TEFF_G</td><td>0.2239432282</td><td>-0.0000467122</td><td>-</td><td>-</td><td>-0.69</td><td>5095</td><td>0.0020</td><td>0.1956</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>Y2</td><td>LOGG_D</td><td>18.5786753232</td><td>-10.6917378985</td><td>1.5217598504</td><td>-</td><td>3.46</td><td>4.20</td><td>-0.0660</td><td>0.5153</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>Y2</td><td>LOGG_G</td><td>-0.168434003</td><td>0.0395075169</td><td>-</td><td>-</td><td>0.98</td><td>2.97</td><td>-0.0950</td><td>0.2638</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>ZR1</td><td>OFFSET</td><td>1.1620</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>1.1620</td><td>4.9400</td><td>WG11-full</td></tr><tr><td>HRT15N</td><td>Lumba</td><td>AL1</td><td>FEH_G</td><td>0.1258188370</td><td>0.0201138850</td><td>0.0890347210</td><td>-</td><td>-1.66</td><td>0.34</td><td>0.1400</td><td>0.1370</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>Lumba</td><td>AL1</td><td>FEH_G</td><td>0.1615605640</td><td>0.0683883570</td><td>0.0985345720</td><td>-</td><td>-1.66</td><td>0.30</td><td>0.1700</td><td>0.1050</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>Lumba</td><td>BA2</td><td>LOGG_D</td><td>2.4205706048</td><td>-2.8519959072</td><td>0.3395505367</td><td>-</td><td>3.46</td><td>4.58</td><td>0.2800</td><td>0.2128</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>Lumba</td><td>BA2</td><td>LOGG_G</td><td>1.2267212441</td><td>-2.678149175</td><td>-</td><td>-</td><td>0.98</td><td>3.35</td><td>0.5900</td><td>0.2151</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>Lumba</td><td>C1</td><td>OFFSET_D</td><td>0.1234004990</td><td>0.0507172730</td><td>-</td><td>-</td><td>-0.43</td><td>0.36</td><td>0.1300</td><td>0.1383</td><td>WG11xmat</td></tr></tbody></table>
Appendix B: Working Group 10 element abundance corrections

<table><caption>Table B.1. Coefficients of WG10 bias corrections.</caption><thead><tr><th>SETUP</th><th>NODE</th><th>ELEMENT</th><th>IP</th><th>a0</th><th>a1</th><th>a2</th><th>a3</th><th>min(IP)</th><th>max(IP)</th><th>MedianA</th><th>σA</th><th>Calibration</th></tr></thead><tbody><tr><td>HRT0</td><td>CAUP</td><td>CA1</td><td>FEH_D</td><td>-0.0128635771</td><td>-0.0853183007</td><td>-</td><td>-</td><td>-2.52</td><td>0.32</td><td>0.0000</td><td>0.1878</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>CAUP</td><td>CA1</td><td>FEH_G</td><td>0.0671735328</td><td>0.0720870430</td><td>-</td><td>-</td><td>-2.00</td><td>0.21</td><td>-0.0100</td><td>0.1762</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>CAUP</td><td>CO1</td><td>FEH_D</td><td>-0.1904706240</td><td>0.0279439500</td><td>-</td><td>-</td><td>-0.30</td><td>0.41</td><td>-0.1800</td><td>0.0902</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>CAUP</td><td>CO1</td><td>FEH_G</td><td>-0.0299998950</td><td>-</td><td>-</td><td>-</td><td>-1.21</td><td>0.21</td><td>-0.0300</td><td>0.0824</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>CAUP</td><td>CR1</td><td>LOGG_D</td><td>-5.6450875166</td><td>2.8491813136</td><td>-0.3506320046</td><td>-</td><td>3.53</td><td>4.59</td><td>0.0800</td><td>0.1470</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>CAUP</td><td>CR1</td><td>FEH_G</td><td>0.0624965243</td><td>-0.0223026185</td><td>-0.0403518382</td><td>-</td><td>-2.62</td><td>0.21</td><td>0.0200</td><td>0.3286</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>CAUP</td><td>FE1</td><td>LOGG_D</td><td>-0.0379078330</td><td>-0.0468408820</td><td>0.0117258380</td><td>-</td><td>0.95</td><td>4.68</td><td>-0.0600</td><td>0.1338</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>CAUP</td><td>FE1</td><td>FEH_G</td><td>-0.0388349210</td><td>0.02757011220</td><td>-0.0078109530</td><td>-</td><td>-2.52</td><td>0.04</td><td>-0.0500</td><td>0.1593</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>CAUP</td><td>MN1</td><td>FEH_D</td><td>-0.2178134436</td><td>-0.1944580752</td><td>-</td><td>-</td><td>-0.25</td><td>0.45</td><td>-0.2200</td><td>0.1458</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>CAUP</td><td>MN1</td><td>FEH_G</td><td>-0.3584931025</td><td>-0.0358944088</td><td>-</td><td>-</td><td>-1.54</td><td>0.21</td><td>-0.3100</td><td>0.1742</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>CAUP</td><td>NI1</td><td>FEH_D</td><td>-0.0322487332</td><td>-0.2028706638</td><td>-</td><td>-</td><td>-0.70</td><td>0.45</td><td>0.0100</td><td>0.1130</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>CAUP</td><td>NI1</td><td>FEH_G</td><td>-0.0539072155</td><td>-0.0685051063</td><td>-</td><td>-</td><td>-1.54</td><td>0.21</td><td>0.0200</td><td>0.1747</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>CAUP</td><td>SC2</td><td>FEH_D</td><td>-0.141620289</td><td>-0.1317874827</td><td>-</td><td>-</td><td>-1.10</td><td>0.45</td><td>-0.1300</td><td>0.1385</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>CAUP</td><td>SC2</td><td>FEH_G</td><td>-0.3906970169</td><td>-0.5386362834</td><td>-0.1670547663</td><td>-</td><td>-1.10</td><td>0.21</td><td>-0.0400</td><td>0.1691</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>CAUP</td><td>TI2</td><td>FEH_D</td><td>-0.1060732326</td><td>-0.0850312307</td><td>-</td><td>-</td><td>-2.52</td><td>0.45</td><td>-0.1100</td><td>0.1078</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>CAUP</td><td>TI2</td><td>FEH_G</td><td>-0.317366324</td><td>-0.3105625844</td><td>-0.0567801729</td><td>-</td><td>-2.62</td><td>0.21</td><td>-0.0800</td><td>0.2249</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>C1</td><td>FEH_D</td><td>0.0732768207</td><td>-0.0491589552</td><td>-</td><td>-</td><td>-0.70</td><td>0.45</td><td>-0.0500</td><td>0.1135</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>C1</td><td>OFFSET_G</td><td>0.2500</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>0.2500</td><td>0.0683</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>CO1</td><td>OFFSET_D</td><td>-0.0500</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-0.0500</td><td>0.1646</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>CO1</td><td>FEH_G</td><td>-0.03130808310</td><td>0.0788521830</td><td>0.1184216920</td><td>-</td><td>-</td><td>-1.26</td><td>0.04</td><td>0.0200</td><td>0.1091</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>CR1</td><td>TEFF_D</td><td>-16.7383167700</td><td>0.0061316870</td><td>-0.0000005546</td><td>-</td><td>4842</td><td>6483</td><td>0.1100</td><td>0.1228</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>CR1</td><td>TEFF_G</td><td>6.7606788150</td><td>-0.0022318690</td><td>0.0000001747</td><td>-</td><td>4423</td><td>6720</td><td>0.0300</td><td>0.2739</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>FE1</td><td>FEH_G</td><td>0.0976131640</td><td>0.0838707160</td><td>0.0123411550</td><td>-</td><td>-2.52</td><td>0.37</td><td>0.0700</td><td>0.2463</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>FE1</td><td>LOGG_D</td><td>4.3500420690</td><td>-2.2274475100</td><td>0.2789431000</td><td>-</td><td>3.45</td><td>4.68</td><td>-0.0700</td><td>0.1282</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>MG1</td><td>FEH</td><td>0.0464074730</td><td>-0.0687944546</td><td>-</td><td>-</td><td>-1.10</td><td>0.45</td><td>0.0600</td><td>0.1221</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>MN1</td><td>FEH</td><td>-0.0721551932</td><td>-0.2434403206</td><td>-0.2944977537</td><td>-</td><td>-1.10</td><td>0.30</td><td>-0.1200</td><td>0.2009</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>MO1</td><td>FEH</td><td>0.4932369290</td><td>1.3317375180</td><td>-0.6803415420</td><td>-3.55216122</td><td>-0.49</td><td>0.35</td><td>0.5000</td><td>3.8600</td><td>WG11-full</td></tr><tr><td>HRT0</td><td>Lumba</td><td>ND2</td><td>OFFSET_D</td><td>0.7200</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>0.7200</td><td>0.1259</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>ND2</td><td>FEH_G</td><td>0.5507316480</td><td>0.6873607070</td><td>0.2871853550</td><td>-</td><td>-</td><td>-1.23</td><td>0.04</td><td>0.0200</td><td>0.1836</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>NI1</td><td>FEH_D</td><td>0.113103971</td><td>0.0412906286</td><td>-</td><td>-</td><td>-0.40</td><td>0.45</td><td>0.1000</td><td>0.1028</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>NI1</td><td>OFFSET_G</td><td>0.1800</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>0.1800</td><td>0.1969</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>SC2</td><td>OFFSET_D</td><td>-0.1100</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-0.1100</td><td>0.1490</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>SC2</td><td>OFFSET_G</td><td>0.0700</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>0.0700</td><td>0.1842</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>V1</td><td>OFFSET_D</td><td>-0.0800</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-0.0800</td><td>0.0283</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>V1</td><td>OFFSET_G</td><td>-0.0400</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-0.0400</td><td>0.0752</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>Y2</td><td>OFFSET_D</td><td>-0.2300</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-0.2300</td><td>0.1245</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>Y2</td><td>OFFSET_G</td><td>-0.0900</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-0.0900</td><td>0.1608</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>ZR1</td><td>FEH</td><td>0.1523604990</td><td>0.5486256480</td><td>1.1509851220</td><td>0.65947002</td><td>-</td><td>-1.25</td><td>0.37</td><td>0.1300</td><td>4.4100</td><td>WG11-full</td></tr><tr><td>HRT0</td><td>Lumba</td><td>AL1</td><td>FEH_D</td><td>0.0598238978</td><td>0.0004466455</td><td>-</td><td>-</td><td>-0.70</td><td>0.45</td><td>-0.0800</td><td>0.0455</td><td>0.1470</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>AL1</td><td>FEH_G</td><td>0.1159365538</td><td>-0.0363255123</td><td>-</td><td>-</td><td>-1.50</td><td>0.21</td><td>0.1800</td><td>0.1879</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>CA1</td><td>FEH_D</td><td>0.1303592641</td><td>0.0529698156</td><td>-</td><td>-</td><td>-0.70</td><td>0.45</td><td>0.1400</td><td>0.1557</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>CA1</td><td>OFFSET_G</td><td>0.0400</td><td>-</td><td>-</td><td>-</td><td>-1.10</td><td>0.21</td><td>0.0400</td><td>0.1886</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>CO1</td><td>FEH_D</td><td>0.1415773330</td><td>0.0838384140</td><td>-0.0796160610</td><td>-</td><td>-0.71</td><td>0.41</td><td>0.1200</td><td>0.1454</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>CO1</td><td>FEH_G</td><td>0.2384163850</td><td>0.2857059710</td><td>0.1121185940</td><td>-</td><td>-1.26</td><td>0.37</td><td>0.0600</td><td>0.2132</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>CR1</td><td>LOGG_D</td><td>3.141860370</td><td>-1.5389358300</td><td>0.1933153520</td><td>-</td><td>3.45</td><td>4.68</td><td>0.0900</td><td>0.1543</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>CR1</td><td>LOGG_G</td><td>0.3495480500</td><td>-0.4913832760</td><td>0.1403916450</td><td>-</td><td>0.95</td><td>3.39</td><td>-0.0200</td><td>0.2645</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>FE1</td><td>LOGG_D</td><td>2.6557655300</td><td>-1.3217719570</td><td>0.1695725040</td><td>-</td><td>3.45</td><td>4.68</td><td>0.1000</td><td>0.1555</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>FE1</td><td>FEH_G</td><td>0.2328755010</td><td>0.1948311820</td><td>0.0523083140</td><td>-</td><td>-2.52</td><td>0.37</td><td>0.0900</td><td>0.2349</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>FE2</td><td>LOGG</td><td>0.6344379240</td><td>-0.2852883300</td><td>0.0442309150</td><td>-</td><td>0.95</td><td>4.68</td><td>-0.0200</td><td>0.2018</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>MG1</td><td>OFFSET_D</td><td>0.1600</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>0.1600</td><td>0.1779</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>MG1</td><td>FEH_G</td><td>-0.0406796642</td><td>-0.3352504432</td><td>-</td><td>-</td><td>-1.10</td><td>0.21</td><td>0.1600</td><td>0.2601</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>MN1</td><td>TEFF_D</td><td>-1.4101857502</td><td>0.0004340610</td><td>-0.0000000316</td><td>-</td><td>4256</td><td>6756</td><td>0.0100</td><td>0.1615</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>MN1</td><td>FEH_G</td><td>0.0285548670</td><td>0.1218215121</td><td>-</td><td>-</td><td>-1.54</td><td>0.21</td><td>-0.0900</td><td>0.1970</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>NI1</td><td>LOGG_D</td><td>6.1505396041</td><td>-3.1638494044</td><td>0.4061924846</td><td>-</td><td>3.53</td><td>4.51</td><td>0.0500</td><td>0.1508</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>NI1</td><td>TEFF_G</td><td>9.0197287067</td><td>-0.0035566944</td><td>0.00000003496</td><td>-</td><td>-1.26</td><td>0.47</td><td>0.0000</td><td>0.2335</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>TI1</td><td>FEH_D</td><td>0.1215496359</td><td>0.0156832702</td><td>-</td><td>-</td><td>-0.70</td><td>0.45</td><td>0.1600</td><td>0.2127</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>TI1</td><td>FEH_G</td><td>-0.207111023</td><td>-0.210711023</td><td>-</td><td>-</td><td>-0.70</td><td>0.00</td><td>0.2000</td><td>0.2336</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>TI2</td><td>FEH_G</td><td>0.3898855087</td><td>-</td><td>-</td><td>-</td><td>-2.62</td><td>0.21</td><td>0.3300</td><td>0.2773</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>TI2</td><td>FEH_D</td><td>0.1096975581</td><td>-0.0688373436</td><td>-0.0399396966</td><td>-</td><td>-2.03</td><td>0.45</td><td>0.1100</td><td>0.2071</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>Y2</td><td>OFFSET_D</td><td>-0.0200</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-0.0200</td><td>0.2140</td><td>WG11xmat</td></tr><tr><td>HRT0</td><td>Lumba</td><td>Y2</td><td>OFFSET_G</td><td>0.0700</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-0.70</td><td>0.1200</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>CAUP</td><td>CA1</td><td>FEH_D</td><td>-0.0987282970</td><td>-0.0744936740</td><td>0.09121791410</td><td>-</td><td>-1.27</td><td>0.20</td><td>0.0700</td><td>0.2044</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>CAUP</td><td>CA1</td><td>FEH_G</td><td>-0.0558260260</td><td>-0.0515666940</td><td>-0.0056638010</td><td>-</td><td>-2.54</td><td>0.32</td><td>-0.0500</td><td>0.1928</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>CAUP</td><td>FE1</td><td>TEFF_D</td><td>1.5395375310</td><td>0.0005183000</td><td>0.0000000444</td><td>-</td><td>4092</td><td>629</td><td>0.0400</td><td>0.1498</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>CAUP</td><td>FE1</td><td>TEFF_G</td><td>6.0155818810</td><td>-0.0025553130</td><td>0.00000002721</td><td>-</td><td>4171</td><td>5132</td><td>0.0400</td><td>0.1189</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>CAUP</td><td>NI1</td><td>TEFF_G</td><td>0.9724628770</td><td>0.0003342880</td><td>0.0000000277</td><td>-</td><td>4092</td><td>5132</td><td>0.0200</td><td>0.1552</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>CAUP</td><td>NI1</td><td>TEFF_G</td><td>9.5562424000</td><td>-0.0041799340</td><td>0.0000004513</td><td>-</td><td>4171</td><td>5132</td><td>-0.0800</td><td>0.1454</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>CAUP</td><td>SC2</td><td>FEH_D</td><td>0.1003669214</td><td>-0.1982793021</td><td>-</td><td>-</td><td>-1.00</td><td>0.00</td><td>-0.0900</td><td>0.1188</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>CAUP</td><td>SC2</td><td>FEH_G</td><td>-0.1855341097</td><td>-0.1870818927</td><td>-</td><td>-</td><td>-1.66</td><td>0.33</td><td>-0.1300</td><td>0.1105</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>CAUP</td><td>SI1</td><td>FEH_D</td><td>0.0506171736</td><td>0.0450048868</td><td>-</td><td>-</td><td>-0.86</td><td>0.49</td><td>0.0500</td><td>0.1275</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>CAUP</td><td>SI1</td><td>FEH_G</td><td>0.0823885330</td><td>0.2563482820</td><td>0.3457082370</td><td>-</td><td>0.86</td><td>0.29</td><td>0.0600</td><td>0.1468</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>AL1</td><td>TEFF_D</td><td>-0.9569700663</td><td>0.0005238327</td><td>-0.0000000558</td><td>-</td><td>5003</td><td>6710</td><td>0.2060</td><td>0.2588</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>AL1</td><td>FEH_G</td><td>0.3162735083</td><td>0.2239841044</td><td>0.0792369502</td><td>-</td><td>-1.66</td><td>0.33</td><td>0.2550</td><td>0.1659</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>BA2</td><td>FEH_D</td><td>0.0985018910</td><td>-0.7698388700</td><td>-0.5755655770</td><td>-0.13481981</td><td>-2.09</td><td>0.32</td><td>0.1310</td><td>2.9850</td><td>WG11-full</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>BA2</td><td>FEH_G</td><td>-0.4055081900</td><td>0.0141792960</td><td>0.14568006990</td><td>0.66517806</td><td>-2.54</td><td>0.17</td><td>0.0560</td><td>0.2650</td><td>WG11-full</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>C1</td><td>OFFSET_D</td><td>0.0800</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-0.0800</td><td>0.1779</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>CA1</td><td>FEH_G</td><td>0.0846544789</td><td>-0.2307559980</td><td>-</td><td>-</td><td>-0.42</td><td>0.33</td><td>0.1400</td><td>0.1920</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>CA1</td><td>OFFSET_D</td><td>0.1740</td><td>-</td><td>-</td><td>-</td><td>-0.56</td><td>0.49</td><td>0.1740</td><td>0.1957</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>CA1</td><td>FEH_G</td><td>0.1069150534</td><td>0.2156591825</td><td>0.1333802684</td><td>-</td><td>-1.66</td><td>0.29</td><td>0.0640</td><td>0.1319</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>CA1</td><td>FEH_D</td><td>0.1945363800</td><td>-0.1662533510</td><td>0.3524026810</td><td>-</td><td>-2.20</td><td>0.36</td><td>0.1980</td><td>0.3100</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>CO1</td><td>FEH_G</td><td>0.2644097580</td><td>-0.0484794770</td><td>-0.1019780170</td><td>-</td><td>-1.66</td><td>0.29</td><td>0.2180</td><td>0.2778</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EU2</td><td>EU2</td><td>OFFSET_D</td><td>0.0590</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>0.0590</td><td>0.1505</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>EU2</td><td>FEH_G</td><td>0.1269190636</td><td>0.1666165730</td><td>-</td><td>-</td><td>-1.58</td><td>0.33</td><td>0.0250</td><td>0.1917</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>FE1</td><td>FEH_D</td><td>0.0462124040</td><td>-0.2231415800</td><td>0.4096522430</td><td>-</td><td>-0.75</td><td>0.36</td><td>0.0790</td><td>0.3726</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>FE1</td><td>FEH_G</td><td>0.0987415140</td><td>0.2070314350</td><td>0.1384381260</td><td>-</td><td>-2.20</td><td>0.36</td><td>0.0810</td><td>0.2919</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>FE1</td><td>FEH_D</td><td>-0.2666048930</td><td>0.0828850200</td><td>-</td><td>-</td><td>-1.20</td><td>0.36</td><td>0.2730</td><td>0.3504</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>FE2</td><td>FEH_G</td><td>0.3398705230</td><td>0.1513853770</td><td>-</td><td>-</td><td>-1.66</td><td>0.29</td><td>0.2750</td><td>0.2321</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>SRI</td><td>OFFSET</td><td>1.6330</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-1.6330</td><td>1.6330</td><td>Scaled Solar</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>TII</td><td>TEFF_D</td><td>17.1293465052</td><td>-0.0064595794</td><td>0.0000006138</td><td>-</td><td>5003</td><td>6300</td><td>0.3030</td><td>0.4986</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>TII</td><td>TEFF_G</td><td>-9.9478595742</td><td>0.0044616249</td><td>-0.0000004934</td><td>-</td><td>4269</td><td>5100</td><td>0.1020</td><td>0.1317</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>V1</td><td>FEH_D</td><td>0.0867662461</td><td>-0.3446519198</td><td>-</td><td>-</td><td>-0.51</td><td>0.49</td><td>0.1100</td><td>0.4483</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>V1</td><td>TEFF_G</td><td>0.2239432282</td><td>-0.0000467122</td><td>-</td><td>-</td><td>-0.69</td><td>0.595</td><td>0.0020</td><td>0.1956</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>Y2</td><td>LOGG_D</td><td>18.5786753232</td><td>-10.6917378985</td><td>1.5217598504</td><td>-</td><td>3.46</td><td>4.20</td><td>-0.0660</td><td>0.5153</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>Y2</td><td>LOGG_G</td><td>-0.168434003</td><td>0.0395075169</td><td>-</td><td>-</td><td>0.98</td><td>2.97</td><td>-0.0950</td><td>0.2638</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>EPINARBO</td><td>ZR1</td><td>OFFSET</td><td>1.1620</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>1.1620</td><td>4.9400</td><td>WG11-full</td></tr><tr><td>HRT15N</td><td>Lumba</td><td>AL1</td><td>FEH_G</td><td>0.1258188370</td><td>0.0201138850</td><td>0.0890347210</td><td>-</td><td>-1.66</td><td>0.34</td><td>0.1400</td><td>0.1370</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>Lumba</td><td>AL1</td><td>FEH_G</td><td>0.1615605640</td><td>0.0683883570</td><td>0.0985345720</td><td>-</td><td>-1.66</td><td>0.30</td><td>0.1700</td><td>0.1050</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>Lumba</td><td>BA2</td><td>LOGG_D</td><td>-2.4205706048</td><td>-2.8519959072</td><td>0.3395505367</td><td>-</td><td>3.46</td><td>4.58</td><td>0.2800</td><td>0.2128</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>Lumba</td><td>BA2</td><td>LOGG_G</td><td>1.2267212441</td><td>-0.2678149175</td><td>-</td><td>-</td><td>0.98</td><td>3.35</td><td>0.5900</td><td>0.2151</td><td>WG11xmat</td></tr><tr><td>HRT15N</td><td>Lumba</td><td>C1</td><td>OFFSET_D</td><td>0.1234004990</td><td>0.0507172730</td><td>-</td><td>-</td><td>-0.43</td><td>0.36</td><td>0.1300</td><td>0.1383</td><td>WG11xmat</td></tr></tbody></table>
<table><caption>Table B.1. continued.</caption><thead><tr><th>SETUP</th><th>NODE</th><th>ELEMENT</th><th>IP</th><th>a0</th><th>a1</th><th>a2</th><th>a3</th><th>min(IP)</th><th>max(IP)</th><th>MedianΔ</th><th>σΔ</th><th>Calibration</th></tr></thead><tbody><tr><td>HR15N</td><td>Lumba</td><td>C1</td><td>OFFSET_G</td><td>0.2393637190</td><td>0.3464880590</td><td>-</td><td>-</td><td>-0.51</td><td>0.29</td><td>0.2200</td><td>0.1388</td><td>WG11xmat</td></tr><tr><td>HR15N</td><td>Lumba</td><td>CA1</td><td>OFFSET_D</td><td>0.1400</td><td>-</td><td>-</td><td>-</td><td>-0.70</td><td>0.49</td><td>0.1400</td><td>0.1595</td><td>WG11xmat</td></tr><tr><td>HR15N</td><td>Lumba</td><td>CA1</td><td>FEH_G</td><td>0.1455244593</td><td>-0.0630665992</td><td>-</td><td>-</td><td>-1.10</td><td>0.33</td><td>0.1800</td><td>0.1932</td><td>WG11xmat</td></tr><tr><td>HR15N</td><td>Lumba</td><td>CO1</td><td>TEFF_D</td><td>-0.7148061500</td><td>0.0001486460</td><td>-</td><td>-</td><td>-413</td><td>6452</td><td>0.1000</td><td>0.1431</td><td>WG11xmat</td></tr><tr><td>HR15N</td><td>Lumba</td><td>CO1</td><td>FEH_G</td><td>0.0176560850</td><td>-0.1413575310</td><td>-0.0389629720</td><td>-</td><td>-1.30</td><td>0.30</td><td>0.0500</td><td>0.0842</td><td>WG11xmat</td></tr><tr><td>HR15N</td><td>Lumba</td><td>EU2</td><td>OFFSET_D</td><td>0.3400</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>0.3400</td><td>0.1436</td><td>WG11xmat</td></tr><tr><td>HR15N</td><td>Lumba</td><td>EU2</td><td>FEH_G</td><td>0.1914570730</td><td>0.2859310470</td><td>0.2835082150</td><td>-</td><td>-1.30</td><td>0.29</td><td>0.1400</td><td>0.1288</td><td>WG11xmat</td></tr><tr><td>HR15N</td><td>Lumba</td><td>N1I</td><td>FEH_D</td><td>0.1008589225</td><td>0.0544224804</td><td>-</td><td>-</td><td>-1.33</td><td>0.49</td><td>0.0900</td><td>0.1769</td><td>WG11xmat</td></tr><tr><td>HR15N</td><td>Lumba</td><td>N1I</td><td>FEH_G</td><td>0.2560589917</td><td>0.0509889047</td><td>-</td><td>-</td><td>-1.66</td><td>0.33</td><td>0.2400</td><td>0.2184</td><td>WG11xmat</td></tr><tr><td>HR15N</td><td>Lumba</td><td>SI1</td><td>LOGG_D</td><td>0.1048324560</td><td>0.0224807643</td><td>-</td><td>-</td><td>3.46</td><td>4.58</td><td>0.1900</td><td>0.1059</td><td>WG11xmat</td></tr><tr><td>HR15N</td><td>Lumba</td><td>SI1</td><td>TEFF_G</td><td>24.1362275043</td><td>-0.0093215520</td><td>0.0000009122</td><td>-</td><td>-</td><td>4400</td><td>5095</td><td>0.4500</td><td>0.4346</td><td>WG11xmat</td></tr><tr><td>HR15N</td><td>Lumba</td><td>TI1</td><td>FEH</td><td>0.0851134142</td><td>-0.0407456089</td><td>-</td><td>-</td><td>-2.03</td><td>0.49</td><td>0.1000</td><td>0.2972</td><td>WG11xmat</td></tr><tr><td>HR21</td><td>CAUP</td><td>AL1</td><td>FEH_D</td><td>-0.1330458850</td><td>0.0140405030</td><td>0.1180994800</td><td>-</td><td>-1.33</td><td>0.45</td><td>0.1200</td><td>0.1356</td><td>WG11xmat</td></tr><tr><td>HR21</td><td>CAUP</td><td>AL1</td><td>FEH_G</td><td>0.0724923910</td><td>0.1917499230</td><td>0.1070101150</td><td>-</td><td>-1.63</td><td>0.21</td><td>-0.0100</td><td>0.1311</td><td>WG11xmat</td></tr><tr><td>HR21</td><td>CAUP</td><td>FE1</td><td>FEH_D</td><td>0.0308106900</td><td>0.2023866500</td><td>0.0894924000</td><td>-</td><td>-0.90</td><td>0.47</td><td>-0.0060</td><td>0.1830</td><td>HR21toHR10-WG11</td></tr><tr><td>HR21</td><td>CAUP</td><td>FE1</td><td>FEH_G</td><td>0.2812608200</td><td>0.4460150900</td><td>0.0927387200</td><td>-</td><td>-0.80</td><td>0.42</td><td>0.1580</td><td>0.2360</td><td>HR21toHR10-WG11</td></tr><tr><td>HR21</td><td>CAUP</td><td>MG1</td><td>OFFSET_D</td><td>-0.0100</td><td>-</td><td>-</td><td>-</td><td>-2.03</td><td>0.45</td><td>-0.0100</td><td>0.1694</td><td>WG11xmat</td></tr><tr><td>HR21</td><td>CAUP</td><td>MG1</td><td>FEH_G</td><td>-0.0149402040</td><td>-0.1185022070</td><td>0.0415395750</td><td>-</td><td>-1.10</td><td>0.21</td><td>0.0700</td><td>0.2260</td><td>WG11xmat</td></tr><tr><td>HR21</td><td>Lumba</td><td>AL1</td><td>FEH_D</td><td>-0.2658367920</td><td>0.0818413460</td><td>0.3999028370</td><td>-</td><td>-0.70</td><td>0.45</td><td>-0.2300</td><td>0.1332</td><td>WG11xmat</td></tr><tr><td>HR21</td><td>Lumba</td><td>AL1</td><td>FEH_G</td><td>-0.2010914430</td><td>0.1827250330</td><td>0.1375634280</td><td>-</td><td>-1.63</td><td>0.21</td><td>-0.2300</td><td>0.1854</td><td>WG11xmat</td></tr><tr><td>HR21</td><td>Lumba</td><td>FE1</td><td>FEH_D</td><td>0.1221244200</td><td>-0.0673754000</td><td>-0.0510338100</td><td>-</td><td>-2.52</td><td>0.45</td><td>0.1320</td><td>0.1570</td><td>HR21toHR10-WG11</td></tr><tr><td>HR21</td><td>Lumba</td><td>FE1</td><td>FEH_G</td><td>0.2208933400</td><td>0.0717466300</td><td>0.0159230300</td><td>-</td><td>-3.11</td><td>0.42</td><td>0.1920</td><td>0.1700</td><td>HR21toHR10-WG11</td></tr><tr><td>HR21</td><td>Lumba</td><td>MG1</td><td>OFFSET_D</td><td>0.1200</td><td>-</td><td>-</td><td>-</td><td>-2.03</td><td>0.45</td><td>0.1200</td><td>0.1850</td><td>WG11xmat</td></tr><tr><td>HR21</td><td>Lumba</td><td>MG1</td><td>FEH_G</td><td>0.0967134805</td><td>-0.0665194907</td><td>0.0651249740</td><td>-</td><td>-1.10</td><td>0.21</td><td>0.2000</td><td>0.2860</td><td>WG11xmat</td></tr><tr><td>HR21</td><td>Lumba</td><td>SI1</td><td>LOGG_D</td><td>-0.3013328157</td><td>0.1152338589</td><td>-</td><td>-</td><td>3.53</td><td>4.59</td><td>0.1800</td><td>0.1160</td><td>WG11xmat</td></tr><tr><td>HR21</td><td>Lumba</td><td>SI1</td><td>FEH_G</td><td>0.5240188932</td><td>0.9555999724</td><td>0.5280106112</td><td>-</td><td>-1.10</td><td>0.00</td><td>0.2000</td><td>0.4609</td><td>WG11xmat</td></tr><tr><td>HR21</td><td>Vilnius</td><td>AL1</td><td>FEH_D</td><td>0.0123871914</td><td>0.0024776950</td><td>-</td><td>-</td><td>-1.33</td><td>0.45</td><td>0.0300</td><td>0.1644</td><td>WG11xmat</td></tr><tr><td>HR21</td><td>Vilnius</td><td>AL1</td><td>FEH_G</td><td>0.3107618178</td><td>0.1954399937</td><td>-</td><td>-</td><td>-1.27</td><td>0.21</td><td>0.1600</td><td>0.1964</td><td>WG11xmat</td></tr><tr><td>HR21</td><td>Vilnius</td><td>CA2</td><td>FEH_D</td><td>0.1236401000</td><td>0.1339087600</td><td>-</td><td>-</td><td>-2.53</td><td>0.42</td><td>0.0420</td><td>0.2710</td><td>HR21toHR10-WG11</td></tr><tr><td>HR21</td><td>Vilnius</td><td>CA2</td><td>FEH_D</td><td>-0.0241594400</td><td>0.2321338100</td><td>0.1195865000</td><td>-</td><td>-0.70</td><td>0.47</td><td>-0.0690</td><td>0.1870</td><td>HR21toHR10-WG11</td></tr><tr><td>HR21</td><td>Vilnius</td><td>FE1</td><td>FEH_D</td><td>0.1630460800</td><td>0.0208094900</td><td>-0.0104126700</td><td>-</td><td>-2.57</td><td>0.47</td><td>0.1330</td><td>0.1330</td><td>HR21toHR10-WG11</td></tr><tr><td>HR21</td><td>Vilnius</td><td>FE1</td><td>FEH_G</td><td>0.5288046000</td><td>0.6799116700</td><td>0.2248112100</td><td>-</td><td>-3.17</td><td>0.93</td><td>0.2890</td><td>0.2610</td><td>HR21toHR10-WG11</td></tr><tr><td>HR21</td><td>Vilnius</td><td>MG1</td><td>OFFSET_D</td><td>0.1580</td><td>-</td><td>-</td><td>-</td><td>-2.57</td><td>0.47</td><td>0.1580</td><td>0.1320</td><td>HR21toHR10-WG11</td></tr><tr><td>HR21</td><td>Vilnius</td><td>MG1</td><td>FEH_G</td><td>0.2158573700</td><td>0.4460271900</td><td>0.5062285700</td><td>-</td><td>-0.30</td><td>0.42</td><td>0.2920</td><td>0.2060</td><td>HR21toHR10-WG11</td></tr><tr><td>HR21</td><td>Vilnius</td><td>SI1</td><td>LOGG_D</td><td>0.0299960908</td><td>0.0267704496</td><td>-</td><td>-</td><td>3.59</td><td>4.60</td><td>0.1200</td><td>0.1307</td><td>WG11xmat</td></tr><tr><td>HR21</td><td>Vilnius</td><td>SI1</td><td>FEH_G</td><td>0.2776062190</td><td>0.4798213770</td><td>0.2179009050</td><td>-</td><td>-1.27</td><td>0.21</td><td>0.0700</td><td>0.2174</td><td>WG11xmat</td></tr><tr><td>HR21</td><td>Vilnius</td><td>TI1</td><td>FEH_D</td><td>0.1499854500</td><td>0.0088722400</td><td>-0.0068887000</td><td>-</td><td>-1.25</td><td>0.47</td><td>0.1480</td><td>0.2650</td><td>HR21toHR10-WG11</td></tr><tr><td>HR21</td><td>Vilnius</td><td>TI1</td><td>FEH_G</td><td>0.3295874000</td><td>0.4103813500</td><td>0.3194012300</td><td>-</td><td>-0.50</td><td>0.42</td><td>0.2430</td><td>0.2430</td><td>HR21toHR10-WG11</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>CA1</td><td>TEFF_D</td><td>-5.6125887540</td><td>0.0017516880</td><td>-0.0000001347</td><td>-</td><td>5030</td><td>6184</td><td>-0.0250</td><td>0.1675</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>CA1</td><td>TEFF_G</td><td>31.6180845900</td><td>-0.0134122070</td><td>0.0000014091</td><td>-</td><td>4585</td><td>5375</td><td>-0.2780</td><td>0.1321</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>CE2</td><td>FEH_G</td><td>-0.2340408971</td><td>-0.6577443268</td><td>-</td><td>-</td><td>-0.10</td><td>0.26</td><td>-0.2980</td><td>0.2162</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>CE2</td><td>FEH_D</td><td>0.0889999659</td><td>0.7001094103</td><td>-</td><td>-</td><td>-0.57</td><td>0.20</td><td>-0.0150</td><td>0.4717</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>CO1</td><td>FEH_D</td><td>-0.1717849057</td><td>0.0075862458</td><td>0.6403065816</td><td>-</td><td>-1.33</td><td>0.33</td><td>-0.0970</td><td>0.3113</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>CO1</td><td>TEFF_G</td><td>45.2018809500</td><td>0.0179687140</td><td>0.0000017819</td><td>-</td><td>4585</td><td>5375</td><td>-0.0230</td><td>0.1880</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>CR1</td><td>LOGG_D</td><td>-0.0278139970</td><td>0.0055499350</td><td>-</td><td>-</td><td>3.52</td><td>4.57</td><td>0.0100</td><td>0.2581</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>CR1</td><td>LOGG_G</td><td>-0.1809654460</td><td>0.0729570610</td><td>-</td><td>-</td><td>2.24</td><td>3.28</td><td>0.0000</td><td>0.1448</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>CR2</td><td>OFFSET</td><td>0.2400</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>0.2400</td><td>-</td><td>WG11-full</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>CU1</td><td>FEH</td><td>0.1247046739</td><td>0.2199904770</td><td>1.6158947945</td><td>5.83671379</td><td>-0.34</td><td>0.32</td><td>0.1590</td><td>8.3430</td><td>WG11-full</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>DY2</td><td>OFFSET</td><td>1.5720</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>1.5720</td><td>-</td><td>Scaled Solar</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>FE1</td><td>FEH_G</td><td>0.0232848290</td><td>-0.0875269150</td><td>-</td><td>-</td><td>-0.11</td><td>0.35</td><td>0.0110</td><td>0.1808</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>FE1</td><td>FEH_D</td><td>-0.0204007620</td><td>-0.2323460920</td><td>-</td><td>-</td><td>-1.30</td><td>0.10</td><td>-0.0080</td><td>0.1993</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>FE2</td><td>FEH</td><td>0.0273802910</td><td>-0.3660831260</td><td>-0.2672870260</td><td>-</td><td>-1.30</td><td>0.38</td><td>0.0340</td><td>0.2372</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>LA2</td><td>FEH</td><td>0.0754013062</td><td>-0.7898668051</td><td>0.5343078971</td><td>2.14124775</td><td>-0.45</td><td>0.39</td><td>0.0910</td><td>2.4200</td><td>WG11-full</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>ND2</td><td>LOGG_D</td><td>-0.3105725040</td><td>0.1304330020</td><td>-</td><td>-</td><td>3.52</td><td>4.41</td><td>0.2590</td><td>0.3008</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>ND2</td><td>LOGG_G</td><td>1.5173952460</td><td>-0.4037327140</td><td>-</td><td>-</td><td>2.24</td><td>3.28</td><td>0.4210</td><td>0.2801</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>N1I</td><td>TEFF</td><td>-0.9498372340</td><td>0.0000613150</td><td>-</td><td>-</td><td>4701</td><td>6117</td><td>-0.6290</td><td>0.2130</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>PR2</td><td>OFFSET</td><td>0.4590</td><td>-</td><td>-</td><td>-</td><td>-</td><td>0</td><td>0.4590</td><td>-</td><td>WG11-full</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>TI1</td><td>OFFSET_D</td><td>0.0980</td><td>-</td><td>-</td><td>-</td><td>3.46</td><td>4.50</td><td>0.0980</td><td>0.2925</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>TI1</td><td>FEH_G</td><td>0.0361210337</td><td>-</td><td>-</td><td>-</td><td>-1.50</td><td>0.28</td><td>-0.0550</td><td>0.2197</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>TI2</td><td>TEFF_D</td><td>1.8107969524</td><td>-0.0000357979</td><td>-</td><td>-</td><td>5700</td><td>6364</td><td>0.0020</td><td>0.2637</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>TI2</td><td>TEFF_G</td><td>0.1834844010</td><td>-0.0000514757</td><td>-</td><td>-</td><td>4521</td><td>5000</td><td>-0.0820</td><td>0.1278</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>Y2</td><td>LOGG</td><td>-1.7901607240</td><td>0.8767585000</td><td>-0.1081206540</td><td>-</td><td>2.24</td><td>4.57</td><td>-0.1990</td><td>0.3211</td><td>WG11xmat</td></tr></tbody></table>

Notes. For each element per node per SETUP, the independent parameter (IP), polynomial fit coefficients, and parameter limits, of the fit of the difference between the WG10 node values and the reference values. The median and σ of the difference is also given. For the IP, _G refers to giant sample, _D refers to dwarf sample.
<table><caption>Table B.1. continued.</caption><thead><tr><th>SETUP</th><th>NODE</th><th>ELEMENT</th><th>IP</th><th>a0</th><th>a1</th><th>a2</th><th>a3</th><th>min(IP)</th><th>max(IP)</th><th>MedianΔ</th><th>σΔ</th><th>Calibration</th></tr></thead><tbody><tr><td>HR15N</td><td>Lumba</td><td>C1</td><td>OFFSET_G</td><td>0.2393637190</td><td>0.3464880590</td><td>-</td><td>-</td><td>-0.51</td><td>0.29</td><td>0.2200</td><td>0.1388</td><td>WG11xmat</td></tr><tr><td>HR15N</td><td>Lumba</td><td>CA1</td><td>OFFSET_D</td><td>0.1400</td><td>-</td><td>-</td><td>-</td><td>-0.70</td><td>0.49</td><td>0.1400</td><td>0.1595</td><td>WG11xmat</td></tr><tr><td>HR15N</td><td>Lumba</td><td>CA1</td><td>FEH_G</td><td>0.1455244593</td><td>-0.0630665992</td><td>-</td><td>-</td><td>-1.10</td><td>0.33</td><td>0.1800</td><td>0.1932</td><td>WG11xmat</td></tr><tr><td>HR15N</td><td>Lumba</td><td>CO1</td><td>TEFF_D</td><td>-0.7148061500</td><td>0.0001486460</td><td>-</td><td>-</td><td>-413</td><td>6452</td><td>0.1000</td><td>0.1431</td><td>WG11xmat</td></tr><tr><td>HR15N</td><td>Lumba</td><td>CO1</td><td>FEH_G</td><td>0.0176560850</td><td>-0.1413575310</td><td>-0.0389629720</td><td>-</td><td>-1.30</td><td>0.30</td><td>0.0500</td><td>0.0842</td><td>WG11xmat</td></tr><tr><td>HR15N</td><td>Lumba</td><td>EU2</td><td>OFFSET_D</td><td>0.3400</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>0.3400</td><td>0.1436</td><td>WG11xmat</td></tr><tr><td>HR15N</td><td>Lumba</td><td>EU2</td><td>FEH_G</td><td>0.1914570730</td><td>0.2859310470</td><td>0.2835082150</td><td>-</td><td>-1.30</td><td>0.29</td><td>0.1400</td><td>0.1288</td><td>WG11xmat</td></tr><tr><td>HR15N</td><td>Lumba</td><td>NI1</td><td>FEH_D</td><td>0.1008589225</td><td>0.0544224804</td><td>-</td><td>-</td><td>-1.33</td><td>0.49</td><td>0.0900</td><td>0.1769</td><td>WG11xmat</td></tr><tr><td>HR15N</td><td>Lumba</td><td>NI1</td><td>FEH_G</td><td>0.2560589917</td><td>0.0509889047</td><td>-</td><td>-</td><td>-1.66</td><td>0.33</td><td>0.2400</td><td>0.2184</td><td>WG11xmat</td></tr><tr><td>HR15N</td><td>Lumba</td><td>SI1</td><td>LOGG_D</td><td>0.1048324560</td><td>0.0224807643</td><td>-</td><td>-</td><td>3.46</td><td>4.58</td><td>0.1900</td><td>0.1059</td><td>WG11xmat</td></tr><tr><td>HR15N</td><td>Lumba</td><td>SI1</td><td>TEFF_G</td><td>24.1362275043</td><td>-0.0093215520</td><td>0.0000009122</td><td>-</td><td>-</td><td>4400</td><td>5095</td><td>0.4500</td><td>0.4346</td><td>WG11xmat</td></tr><tr><td>HR15N</td><td>Lumba</td><td>TI1</td><td>FEH</td><td>0.0851134142</td><td>-0.0407456089</td><td>-</td><td>-</td><td>-2.03</td><td>0.49</td><td>0.1000</td><td>0.2972</td><td>WG11xmat</td></tr><tr><td>HR21</td><td>CAUP</td><td>AL1</td><td>FEH_D</td><td>-0.1330458850</td><td>0.0140405030</td><td>0.1180994800</td><td>-</td><td>-1.33</td><td>0.45</td><td>0.1200</td><td>0.1356</td><td>WG11xmat</td></tr><tr><td>HR21</td><td>CAUP</td><td>AL1</td><td>FEH_G</td><td>0.0724923910</td><td>0.1917499230</td><td>0.1070101150</td><td>-</td><td>-1.63</td><td>0.21</td><td>-0.0100</td><td>0.1311</td><td>WG11xmat</td></tr><tr><td>HR21</td><td>CAUP</td><td>FE1</td><td>FEH_D</td><td>0.0308106900</td><td>0.2023866500</td><td>0.0894924000</td><td>-</td><td>-0.90</td><td>0.47</td><td>-0.0060</td><td>0.1830</td><td>HR21toHR10-WG11</td></tr><tr><td>HR21</td><td>CAUP</td><td>FE1</td><td>FEH_G</td><td>0.2812608200</td><td>0.4460150900</td><td>0.0927387200</td><td>-</td><td>-0.80</td><td>0.42</td><td>0.1580</td><td>0.2360</td><td>HR21toHR10-WG11</td></tr><tr><td>HR21</td><td>CAUP</td><td>MG1</td><td>OFFSET_D</td><td>-0.0100</td><td>-</td><td>-</td><td>-</td><td>-2.03</td><td>0.45</td><td>-0.0100</td><td>0.1694</td><td>WG11xmat</td></tr><tr><td>HR21</td><td>CAUP</td><td>MG1</td><td>FEH_G</td><td>-0.0149402040</td><td>-0.1185022070</td><td>0.0415395750</td><td>-</td><td>-1.10</td><td>0.21</td><td>0.0700</td><td>0.2260</td><td>WG11xmat</td></tr><tr><td>HR21</td><td>Lumba</td><td>AL1</td><td>FEH_D</td><td>-0.2658367920</td><td>0.0818413460</td><td>0.3999028370</td><td>-</td><td>-0.70</td><td>0.45</td><td>-0.2300</td><td>0.1332</td><td>WG11xmat</td></tr><tr><td>HR21</td><td>Lumba</td><td>AL1</td><td>FEH_G</td><td>-0.2010914430</td><td>0.1827250330</td><td>0.1375634280</td><td>-</td><td>-1.63</td><td>0.21</td><td>-0.2300</td><td>0.1854</td><td>WG11xmat</td></tr><tr><td>HR21</td><td>Lumba</td><td>FE1</td><td>FEH_D</td><td>0.1221244200</td><td>-0.0673754000</td><td>-0.0510338100</td><td>-</td><td>-2.52</td><td>0.45</td><td>0.1320</td><td>0.1570</td><td>HR21toHR10-WG11</td></tr><tr><td>HR21</td><td>Lumba</td><td>FE1</td><td>FEH_G</td><td>0.2208933400</td><td>0.0717466300</td><td>0.0159230300</td><td>-</td><td>-3.11</td><td>0.42</td><td>0.1920</td><td>0.1700</td><td>HR21toHR10-WG11</td></tr><tr><td>HR21</td><td>Lumba</td><td>MG1</td><td>OFFSET_D</td><td>0.1200</td><td>-</td><td>-</td><td>-</td><td>-2.03</td><td>0.45</td><td>0.1200</td><td>0.1850</td><td>WG11xmat</td></tr><tr><td>HR21</td><td>Lumba</td><td>MG1</td><td>FEH_G</td><td>0.0967134805</td><td>-0.0665194907</td><td>0.0651249740</td><td>-</td><td>-1.10</td><td>0.21</td><td>0.2000</td><td>0.2860</td><td>WG11xmat</td></tr><tr><td>HR21</td><td>Lumba</td><td>SI1</td><td>LOGG_D</td><td>-0.3013328157</td><td>0.1152338589</td><td>-</td><td>-</td><td>3.53</td><td>4.59</td><td>0.1800</td><td>0.1160</td><td>WG11xmat</td></tr><tr><td>HR21</td><td>Lumba</td><td>SI1</td><td>FEH_G</td><td>0.5240188932</td><td>0.9555999724</td><td>0.5280106112</td><td>-</td><td>-1.10</td><td>0.00</td><td>0.2000</td><td>0.4609</td><td>WG11xmat</td></tr><tr><td>HR21</td><td>Vilnius</td><td>AL1</td><td>FEH_D</td><td>0.0123871914</td><td>0.0024776950</td><td>-</td><td>-</td><td>-1.33</td><td>0.45</td><td>0.0300</td><td>0.1644</td><td>WG11xmat</td></tr><tr><td>HR21</td><td>Vilnius</td><td>AL1</td><td>FEH_G</td><td>0.3107618178</td><td>0.1954399937</td><td>-</td><td>-</td><td>-1.27</td><td>0.21</td><td>0.1600</td><td>0.1964</td><td>WG11xmat</td></tr><tr><td>HR21</td><td>Vilnius</td><td>CA2</td><td>FEH_D</td><td>0.1236401000</td><td>0.1339087600</td><td>-</td><td>-</td><td>-2.53</td><td>0.42</td><td>0.0420</td><td>0.2710</td><td>HR21toHR10-WG11</td></tr><tr><td>HR21</td><td>Vilnius</td><td>CA2</td><td>FEH_D</td><td>-0.0241594400</td><td>0.2321338100</td><td>0.1195865000</td><td>-</td><td>-0.70</td><td>0.47</td><td>-0.0690</td><td>0.1870</td><td>HR21toHR10-WG11</td></tr><tr><td>HR21</td><td>Vilnius</td><td>FE1</td><td>FEH_D</td><td>0.1630460800</td><td>0.0208094900</td><td>-0.0104126700</td><td>-</td><td>-2.57</td><td>0.47</td><td>0.1330</td><td>0.1330</td><td>HR21toHR10-WG11</td></tr><tr><td>HR21</td><td>Vilnius</td><td>FE1</td><td>FEH_G</td><td>0.5288046000</td><td>0.6799116700</td><td>0.2248112100</td><td>-</td><td>-3.17</td><td>0.93</td><td>0.2890</td><td>0.2610</td><td>HR21toHR10-WG11</td></tr><tr><td>HR21</td><td>Vilnius</td><td>MG1</td><td>OFFSET_D</td><td>0.1580</td><td>-</td><td>-</td><td>-</td><td>-2.57</td><td>0.47</td><td>0.1580</td><td>0.1320</td><td>HR21toHR10-WG11</td></tr><tr><td>HR21</td><td>Vilnius</td><td>MG1</td><td>FEH_G</td><td>0.2158573700</td><td>0.4460271900</td><td>0.5062285700</td><td>-</td><td>-0.30</td><td>0.42</td><td>0.2920</td><td>0.2060</td><td>HR21toHR10-WG11</td></tr><tr><td>HR21</td><td>Vilnius</td><td>SI1</td><td>LOGG_D</td><td>0.0299960908</td><td>0.0267704496</td><td>-</td><td>-</td><td>3.59</td><td>4.60</td><td>0.1200</td><td>0.1307</td><td>WG11xmat</td></tr><tr><td>HR21</td><td>Vilnius</td><td>SI1</td><td>FEH_G</td><td>0.2776062190</td><td>0.4798213770</td><td>0.2179009050</td><td>-</td><td>-1.27</td><td>0.21</td><td>0.0700</td><td>0.2174</td><td>WG11xmat</td></tr><tr><td>HR21</td><td>Vilnius</td><td>TI1</td><td>FEH_D</td><td>0.1499854500</td><td>0.0088722400</td><td>-0.0068887000</td><td>-</td><td>-1.25</td><td>0.47</td><td>0.1480</td><td>0.2650</td><td>HR21toHR10-WG11</td></tr><tr><td>HR21</td><td>Vilnius</td><td>TI1</td><td>FEH_G</td><td>0.3295874000</td><td>0.4103813500</td><td>0.3194012300</td><td>-</td><td>-0.50</td><td>0.42</td><td>0.2430</td><td>0.2430</td><td>HR21toHR10-WG11</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>CA1</td><td>TEFF_D</td><td>-5.6125887540</td><td>0.0017516880</td><td>-0.0000001347</td><td>-</td><td>5030</td><td>6184</td><td>-0.0250</td><td>0.1675</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>CA1</td><td>TEFF_G</td><td>31.6180845900</td><td>-0.0134122070</td><td>0.0000014091</td><td>-</td><td>4585</td><td>5375</td><td>-0.2780</td><td>0.1321</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>CE2</td><td>FEH_G</td><td>-0.2340408971</td><td>-0.6577443268</td><td>-</td><td>-</td><td>-0.10</td><td>0.26</td><td>-0.2980</td><td>0.2162</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>CE2</td><td>FEH_D</td><td>0.0889999659</td><td>0.7001094103</td><td>-</td><td>-</td><td>-0.57</td><td>0.20</td><td>-0.0150</td><td>0.4717</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>CO1</td><td>FEH_D</td><td>-0.1717849057</td><td>0.0075862458</td><td>0.6403065816</td><td>-</td><td>-1.33</td><td>0.33</td><td>-0.0970</td><td>0.3113</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>CO1</td><td>TEFF_G</td><td>45.2018809500</td><td>0.0179687140</td><td>0.0000017819</td><td>-</td><td>4585</td><td>5375</td><td>-0.0230</td><td>0.1880</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>CR1</td><td>LOGG_D</td><td>-0.0278139970</td><td>0.0055499350</td><td>-</td><td>-</td><td>3.52</td><td>4.57</td><td>0.0100</td><td>0.2581</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>CR1</td><td>LOGG_G</td><td>-0.1809654460</td><td>0.0729570610</td><td>-</td><td>-</td><td>2.24</td><td>3.28</td><td>0.0000</td><td>0.1448</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>CR2</td><td>OFFSET</td><td>0.2400</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>0.2400</td><td>-</td><td>WG11-full</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>CU1</td><td>FEH</td><td>0.1247046739</td><td>0.2199904770</td><td>1.6158947945</td><td>5.83671379</td><td>-0.34</td><td>0.32</td><td>0.1590</td><td>8.3430</td><td>WG11-full</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>DY2</td><td>OFFSET</td><td>1.5720</td><td>-</td><td>-</td><td>-</td><td>-</td><td>-</td><td>1.5720</td><td>-</td><td>Scaled Solar</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>FE1</td><td>FEH_G</td><td>0.0232848290</td><td>-0.0875269150</td><td>-</td><td>-</td><td>-0.11</td><td>0.35</td><td>0.0110</td><td>0.1808</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>FE1</td><td>FEH_D</td><td>-0.0204007620</td><td>-0.2323460920</td><td>-</td><td>-</td><td>-1.30</td><td>0.10</td><td>-0.0080</td><td>0.1993</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>FE2</td><td>FEH</td><td>0.0273802910</td><td>-0.3660831260</td><td>-0.2672870260</td><td>-</td><td>-1.30</td><td>0.38</td><td>0.0340</td><td>0.2372</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>LA2</td><td>FEH</td><td>0.0754013062</td><td>-0.7898668051</td><td>0.5343078971</td><td>2.14124775</td><td>-0.45</td><td>0.39</td><td>0.0910</td><td>2.4200</td><td>WG11-full</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>ND2</td><td>LOGG_D</td><td>-0.3105725040</td><td>0.1304330020</td><td>-</td><td>-</td><td>3.52</td><td>4.41</td><td>0.2590</td><td>0.3008</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>ND2</td><td>LOGG_G</td><td>1.5173952460</td><td>-0.4037327140</td><td>-</td><td>-</td><td>2.24</td><td>3.28</td><td>0.4210</td><td>0.2801</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>NI1</td><td>TEFF</td><td>-0.9498372340</td><td>0.0000613150</td><td>-</td><td>-</td><td>4701</td><td>6117</td><td>-0.6290</td><td>0.2130</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>PR2</td><td>OFFSET</td><td>0.4590</td><td>-</td><td>-</td><td>-</td><td>-</td><td>0</td><td>0.4590</td><td>-</td><td>WG11-full</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>TI1</td><td>OFFSET_D</td><td>0.0980</td><td>-</td><td>-</td><td>-</td><td>3.46</td><td>4.50</td><td>0.0980</td><td>0.2925</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>TI1</td><td>FEH_G</td><td>0.0361210337</td><td>-</td><td>-</td><td>-</td><td>-1.50</td><td>0.28</td><td>-0.0550</td><td>0.2197</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>TI2</td><td>TEFF_D</td><td>1.8107969524</td><td>-0.0000357979</td><td>-</td><td>-</td><td>5700</td><td>6364</td><td>0.0020</td><td>0.2637</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>TI2</td><td>TEFF_G</td><td>0.1834844010</td><td>-0.0000514757</td><td>-</td><td>-</td><td>4521</td><td>5000</td><td>-0.0820</td><td>0.1278</td><td>WG11xmat</td></tr><tr><td>HR9B</td><td>EPINARBO</td><td>Y2</td><td>LOGG</td><td>-1.7901607240</td><td>0.8767585000</td><td>-0.1081206540</td><td>-</td><td>2.24</td><td>4.57</td><td>-0.1990</td><td>0.3211</td><td>WG11xmat</td></tr></tbody></table>

Notes. For each element per node per SETUP, the independent parameter (IP), polynomial fit coefficients, and parameter limits, of the fit of the difference between the WG10 node values and the reference values. The median and σ of the difference is also given. For the IP, _G refers to giant sample, _D refers to dwarf sample.