<table><caption>Table C2
The Mean (⟨Δ⟩), Median (Δ̃), and Standard Deviation (σ) of the Balrog griz Magnitude Responses Binned in Injection Magnitude for the y3-deep Sample</caption><thead><tr><th>True Mag</th><th>⟨Δg⟩<br>(mag)</th><th>Δ̃g<br>(mag)</th><th>σ<sub>g</sub><br>(mag)</th><th>⟨Δr⟩<br>(mag)</th><th>Δ̃r<br>(mag)</th><th>σ<sub>r</sub><br>(mag)</th><th>⟨Δi⟩<br>(mag)</th><th>Δ̃i<br>(mag)</th><th>σ<sub>i</sub><br>(mag)</th><th>⟨Δz⟩<br>(mag)</th><th>Δ̃z<br>(mag)</th><th>σ<sub>z</sub><br>(mag)</th></tr></thead><tbody><tr><td>18.00</td><td>-0.066</td><td>-0.039</td><td>0.081</td><td>-0.055</td><td>-0.035</td><td>0.081</td><td>-0.048</td><td>-0.029</td><td>0.087</td><td>-0.043</td><td>-0.024</td><td>0.076</td></tr><tr><td>18.25</td><td>-0.063</td><td>-0.042</td><td>0.101</td><td>-0.052</td><td>-0.033</td><td>0.084</td><td>-0.042</td><td>-0.024</td><td>0.069</td><td>-0.039</td><td>-0.020</td><td>0.076</td></tr><tr><td>18.50</td><td>-0.059</td><td>-0.036</td><td>0.077</td><td>-0.046</td><td>-0.028</td><td>0.079</td><td>-0.039</td><td>-0.019</td><td>0.079</td><td>-0.040</td><td>-0.020</td><td>0.083</td></tr><tr><td>18.75</td><td>-0.055</td><td>-0.036</td><td>0.078</td><td>-0.039</td><td>-0.020</td><td>0.076</td><td>-0.039</td><td>-0.020</td><td>0.077</td><td>-0.034</td><td>-0.014</td><td>0.083</td></tr><tr><td>19.00</td><td>-0.055</td><td>-0.033</td><td>0.083</td><td>-0.041</td><td>-0.021</td><td>0.077</td><td>-0.035</td><td>-0.015</td><td>0.086</td><td>-0.031</td><td>-0.010</td><td>0.090</td></tr><tr><td>19.25</td><td>-0.044</td><td>-0.023</td><td>0.084</td><td>-0.036</td><td>-0.018</td><td>0.079</td><td>-0.031</td><td>-0.011</td><td>0.085</td><td>-0.026</td><td>-0.006</td><td>0.101</td></tr><tr><td>19.50</td><td>-0.040</td><td>-0.022</td><td>0.078</td><td>-0.033</td><td>-0.013</td><td>0.087</td><td>-0.027</td><td>-0.006</td><td>0.096</td><td>-0.022</td><td>-0.002</td><td>0.105</td></tr><tr><td>19.75</td><td>-0.040</td><td>-0.020</td><td>0.085</td><td>-0.030</td><td>-0.009</td><td>0.088</td><td>-0.025</td><td>-0.003</td><td>0.109</td><td>-0.019</td><td>0.002</td><td>0.115</td></tr><tr><td>20.00</td><td>-0.035</td><td>-0.015</td><td>0.078</td><td>-0.026</td><td>-0.006</td><td>0.105</td><td>-0.022</td><td>0.000</td><td>0.110</td><td>-0.016</td><td>0.005</td><td>0.125</td></tr><tr><td>20.25</td><td>-0.035</td><td>-0.015</td><td>0.098</td><td>-0.024</td><td>-0.003</td><td>0.105</td><td>-0.020</td><td>0.003</td><td>0.119</td><td>-0.012</td><td>0.009</td><td>0.134</td></tr><tr><td>20.50</td><td>-0.032</td><td>-0.012</td><td>0.090</td><td>-0.023</td><td>0.000</td><td>0.109</td><td>-0.016</td><td>0.006</td><td>0.126</td><td>-0.008</td><td>0.013</td><td>0.153</td></tr><tr><td>20.75</td><td>-0.030</td><td>-0.009</td><td>0.110</td><td>-0.020</td><td>0.002</td><td>0.122</td><td>-0.013</td><td>0.009</td><td>0.145</td><td>-0.003</td><td>0.017</td><td>0.161</td></tr><tr><td>21.00</td><td>-0.027</td><td>-0.006</td><td>0.107</td><td>-0.018</td><td>0.005</td><td>0.133</td><td>-0.010</td><td>0.013</td><td>0.155</td><td>0.001</td><td>0.021</td><td>0.174</td></tr><tr><td>21.25</td><td>-0.026</td><td>-0.005</td><td>0.116</td><td>-0.016</td><td>0.008</td><td>0.148</td><td>-0.007</td><td>0.017</td><td>0.163</td><td>0.003</td><td>0.025</td><td>0.194</td></tr><tr><td>21.50</td><td>-0.023</td><td>-0.002</td><td>0.127</td><td>-0.014</td><td>0.010</td><td>0.157</td><td>-0.005</td><td>0.020</td><td>0.176</td><td>0.006</td><td>0.028</td><td>0.211</td></tr><tr><td>21.75</td><td>-0.022</td><td>0.000</td><td>0.147</td><td>-0.012</td><td>0.014</td><td>0.171</td><td>-0.002</td><td>0.023</td><td>0.189</td><td>0.008</td><td>0.031</td><td>0.228</td></tr><tr><td>22.00</td><td>-0.020</td><td>0.002</td><td>0.154</td><td>-0.010</td><td>0.017</td><td>0.181</td><td>-0.001</td><td>0.026</td><td>0.203</td><td>0.011</td><td>0.034</td><td>0.254</td></tr><tr><td>22.25</td><td>-0.019</td><td>0.005</td><td>0.171</td><td>-0.009</td><td>0.020</td><td>0.192</td><td>0.001</td><td>0.030</td><td>0.222</td><td>0.015</td><td>0.036</td><td>0.291</td></tr><tr><td>22.50</td><td>-0.017</td><td>0.007</td><td>0.187</td><td>-0.007</td><td>0.024</td><td>0.212</td><td>0.003</td><td>0.033</td><td>0.248</td><td>0.020</td><td>0.039</td><td>0.339</td></tr><tr><td>22.75</td><td>-0.017</td><td>0.010</td><td>0.200</td><td>-0.005</td><td>0.028</td><td>0.231</td><td>0.005</td><td>0.036</td><td>0.279</td><td>0.022</td><td>0.037</td><td>0.403</td></tr><tr><td>23.00</td><td>-0.014</td><td>0.013</td><td>0.220</td><td>-0.004</td><td>0.031</td><td>0.259</td><td>0.004</td><td>0.036</td><td>0.314</td><td>0.024</td><td>0.030</td><td>0.496</td></tr><tr><td>23.25</td><td>-0.012</td><td>0.017</td><td>0.247</td><td>-0.004</td><td>0.034</td><td>0.293</td><td>-0.002</td><td>0.031</td><td>0.355</td><td>0.028</td><td>0.014</td><td>0.663</td></tr><tr><td>23.50</td><td>-0.011</td><td>0.020</td><td>0.279</td><td>-0.008</td><td>0.033</td><td>0.329</td><td>-0.023</td><td>0.013</td><td>0.391</td><td>0.037</td><td>-0.013</td><td>0.916</td></tr><tr><td>23.75</td><td>-0.009</td><td>0.022</td><td>0.323</td><td>-0.023</td><td>0.021</td><td>0.369</td><td>-0.064</td><td>-0.026</td><td>0.442</td><td>0.069</td><td>-0.053</td><td>1.312</td></tr><tr><td>24.00</td><td>-0.009</td><td>0.020</td><td>0.383</td><td>-0.055</td><td>-0.007</td><td>0.413</td><td>-0.132</td><td>-0.091</td><td>0.528</td><td>0.142</td><td>-0.115</td><td>1.874</td></tr><tr><td>24.25</td><td>-0.012</td><td>0.014</td><td>0.463</td><td>-0.108</td><td>-0.057</td><td>0.492</td><td>-0.233</td><td>-0.194</td><td>0.713</td><td>0.232</td><td>-0.217</td><td>2.463</td></tr></tbody></table>

Note. The quoted magnitudes correspond to the left bin edge. Simple Gaussian statistics do not fully capture the complexity of the responses—see Figure 16.

<table><caption>Table C3
The Mean (⟨Δ⟩), Median (Δ̃), and Standard Deviation (σ) of the Balrog g-r, r-i, and i-z Color Responses Binned in Injection Color for the δ-stars Sample</caption><thead><tr><th>True Color</th><th>⟨g-r⟩<br>(mag)</th><th>g̃-r̃<br>(mag)</th><th>σ<sub>g-r</sub><br>(mag)</th><th>⟨r-i⟩<br>(mag)</th><th>r̃-ĩ<br>(mag)</th><th>σ<sub>r-i</sub><br>(mag)</th><th>⟨i-z⟩<br>(mag)</th><th>ĩ-z̃<br>(mag)</th><th>σ<sub>i-z</sub><br>(mag)</th></tr></thead><tbody><tr><td>-0.2</td><td>-0.006</td><td>-0.003</td><td>0.082</td><td>-0.006</td><td>-0.003</td><td>0.111</td><td>0.000</td><td>-0.003</td><td>0.156</td></tr><tr><td>-0.1</td><td>-0.004</td><td>-0.002</td><td>0.098</td><td>-0.007</td><td>-0.003</td><td>0.102</td><td>-0.002</td><td>-0.002</td><td>0.114</td></tr><tr><td>0.0</td><td>-0.003</td><td>-0.002</td><td>0.092</td><td>-0.004</td><td>-0.002</td><td>0.074</td><td>-0.002</td><td>-0.001</td><td>0.091</td></tr><tr><td>0.1</td><td>-0.004</td><td>-0.003</td><td>0.09</td><td>-0.004</td><td>-0.002</td><td>0.078</td><td>-0.002</td><td>-0.001</td><td>0.11</td></tr><tr><td>0.2</td><td>-0.002</td><td>-0.002</td><td>0.074</td><td>-0.003</td><td>-0.002</td><td>0.09</td><td>-0.002</td><td>-0.001</td><td>0.111</td></tr><tr><td>0.3</td><td>-0.001</td><td>-0.002</td><td>0.077</td><td>-0.002</td><td>-0.002</td><td>0.097</td><td>-0.002</td><td>-0.001</td><td>0.101</td></tr><tr><td>0.4</td><td>-0.001</td><td>-0.001</td><td>0.085</td><td>-0.001</td><td>-0.002</td><td>0.096</td><td>-0.002</td><td>-0.001</td><td>0.092</td></tr><tr><td>0.5</td><td>0.000</td><td>-0.001</td><td>0.09</td><td>0.000</td><td>-0.001</td><td>0.094</td><td>-0.001</td><td>-0.001</td><td>0.087</td></tr><tr><td>0.6</td><td>0.000</td><td>-0.001</td><td>0.103</td><td>0.001</td><td>-0.001</td><td>0.091</td><td>0.000</td><td>-0.001</td><td>0.083</td></tr><tr><td>0.7</td><td>-0.001</td><td>-0.001</td><td>0.109</td><td>0.001</td><td>-0.001</td><td>0.088</td><td>0.001</td><td>-0.001</td><td>0.078</td></tr><tr><td>0.8</td><td>-0.002</td><td>-0.001</td><td>0.113</td><td>0.002</td><td>-0.001</td><td>0.092</td><td>0.001</td><td>0.000</td><td>0.075</td></tr><tr><td>0.9</td><td>-0.003</td><td>-0.001</td><td>0.126</td><td>0.002</td><td>-0.001</td><td>0.097</td><td>0.001</td><td>0.000</td><td>0.081</td></tr><tr><td>1.0</td><td>-0.006</td><td>-0.001</td><td>0.131</td><td>0.002</td><td>-0.001</td><td>0.101</td><td>0.004</td><td>0.001</td><td>0.084</td></tr><tr><td>1.1</td><td>-0.010</td><td>-0.002</td><td>0.142</td><td>0.003</td><td>-0.001</td><td>0.106</td><td>0.003</td><td>0.001</td><td>0.078</td></tr><tr><td>1.2</td><td>-0.017</td><td>-0.003</td><td>0.154</td><td>0.002</td><td>-0.001</td><td>0.112</td><td>0.020</td><td>0.001</td><td>0.073</td></tr><tr><td>1.3</td><td>-0.021</td><td>-0.003</td><td>0.155</td><td>0.002</td><td>0.000</td><td>0.116</td><td>-0.024</td><td>0.000</td><td>0.177</td></tr><tr><td>1.4</td><td>-0.027</td><td>-0.004</td><td>0.17</td><td>0.000</td><td>0.001</td><td>0.123</td><td>0.006</td><td>-0.003</td><td>0.119</td></tr><tr><td>1.5</td><td>-0.044</td><td>-0.01</td><td>0.208</td><td>0.000</td><td>0.000</td><td>0.129</td><td>-0.008</td><td>-0.008</td><td>0.007</td></tr><tr><td>1.6</td><td>-0.061</td><td>-0.017</td><td>0.24</td><td>0.000</td><td>0.000</td><td>0.137</td><td>...</td><td>...</td><td>...</td></tr><tr><td>1.7</td><td>-0.076</td><td>-0.026</td><td>0.265</td><td>-0.004</td><td>-0.001</td><td>0.138</td><td>...</td><td>...</td><td>...</td></tr></tbody></table>

Note. The quoted colors correspond to the left bin edge. Simple Gaussian statistics do not fully capture the complexity of the responses—see Figure 14.
<table><caption>**Table C4**
The Mean (⟨Δ⟩), Median (Δ̃), and Standard Deviation (σ) of the Balrog g - r, r - i, and i - z Color Responses Binned in Injection Color for the y3-deep Sample</caption><thead><tr><th>True Color</th><th>⟨g - r⟩<br>(mag)</th><th>⟨g̃ - r̃⟩<br>(mag)</th><th>σ<sub>g-r</sub><br>(mag)</th><th>⟨r - i⟩<br>(mag)</th><th>⟨i - z⟩<br>(mag)</th><th>σ<sub>r-i</sub><br>(mag)</th><th>⟨i - z⟩<br>(mag)</th><th>σ<sub>i-z</sub><br>(mag)</th></tr></thead><tbody><tr><td>-0.2</td><td>0.081</td><td>0.053</td><td>0.211</td><td>0.079</td><td>0.043</td><td>0.216</td><td>0.092</td><td>0.047</td><td>0.239</td></tr><tr><td>-0.1</td><td>0.047</td><td>0.030</td><td>0.192</td><td>0.053</td><td>0.032</td><td>0.201</td><td>0.062</td><td>0.030</td><td>0.213</td></tr><tr><td>0.0</td><td>0.026</td><td>0.016</td><td>0.182</td><td>0.028</td><td>0.013</td><td>0.182</td><td>0.030</td><td>0.009</td><td>0.177</td></tr><tr><td>0.1</td><td>0.012</td><td>0.006</td><td>0.179</td><td>0.011</td><td>0.002</td><td>0.155</td><td>0.019</td><td>0.004</td><td>0.163</td></tr><tr><td>0.2</td><td>0.002</td><td>-0.002</td><td>0.178</td><td>0.004</td><td>0.000</td><td>0.140</td><td>0.011</td><td>0.001</td><td>0.145</td></tr><tr><td>0.3</td><td>-0.009</td><td>-0.006</td><td>0.169</td><td>0.001</td><td>-0.001</td><td>0.140</td><td>0.007</td><td>0.000</td><td>0.134</td></tr><tr><td>0.4</td><td>-0.015</td><td>-0.008</td><td>0.161</td><td>-0.003</td><td>-0.001</td><td>0.139</td><td>0.004</td><td>0.000</td><td>0.141</td></tr><tr><td>0.5</td><td>-0.019</td><td>-0.009</td><td>0.158</td><td>-0.007</td><td>-0.003</td><td>0.140</td><td>0.001</td><td>-0.001</td><td>0.160</td></tr><tr><td>0.6</td><td>-0.024</td><td>-0.010</td><td>0.157</td><td>-0.012</td><td>-0.005</td><td>0.146</td><td>-0.004</td><td>-0.003</td><td>0.161</td></tr><tr><td>0.7</td><td>-0.028</td><td>-0.011</td><td>0.158</td><td>-0.015</td><td>-0.007</td><td>0.147</td><td>-0.009</td><td>-0.005</td><td>0.159</td></tr><tr><td>0.8</td><td>-0.031</td><td>-0.011</td><td>0.159</td><td>-0.018</td><td>-0.007</td><td>0.146</td><td>-0.012</td><td>-0.007</td><td>0.161</td></tr><tr><td>0.9</td><td>-0.036</td><td>-0.011</td><td>0.162</td><td>-0.022</td><td>-0.008</td><td>0.152</td><td>-0.016</td><td>-0.009</td><td>0.171</td></tr><tr><td>1.0</td><td>-0.041</td><td>-0.011</td><td>0.167</td><td>-0.026</td><td>-0.010</td><td>0.161</td><td>-0.019</td><td>-0.011</td><td>0.176</td></tr><tr><td>1.1</td><td>-0.046</td><td>-0.011</td><td>0.173</td><td>-0.029</td><td>-0.012</td><td>0.170</td><td>-0.031</td><td>-0.016</td><td>0.193</td></tr><tr><td>1.2</td><td>-0.051</td><td>-0.010</td><td>0.184</td><td>-0.035</td><td>-0.013</td><td>0.178</td><td>-0.053</td><td>-0.024</td><td>0.210</td></tr><tr><td>1.3</td><td>-0.059</td><td>-0.011</td><td>0.194</td><td>-0.071</td><td>-0.030</td><td>0.221</td><td>-0.049</td><td>-0.024</td><td>0.215</td></tr><tr><td>1.4</td><td>-0.069</td><td>-0.013</td><td>0.210</td><td>-0.149</td><td>-0.091</td><td>0.276</td><td>-0.054</td><td>-0.018</td><td>0.223</td></tr><tr><td>1.5</td><td>-0.074</td><td>-0.015</td><td>0.222</td><td>-0.171</td><td>-0.105</td><td>0.288</td><td>-0.076</td><td>-0.028</td><td>0.236</td></tr><tr><td>1.6</td><td>-0.070</td><td>-0.016</td><td>0.224</td><td>-0.183</td><td>-0.112</td><td>0.300</td><td>-0.075</td><td>-0.015</td><td>0.220</td></tr><tr><td>1.7</td><td>-0.066</td><td>-0.016</td><td>0.224</td><td>-0.206</td><td>-0.126</td><td>0.314</td><td>-0.050</td><td>-0.007</td><td>0.240</td></tr><tr><td>1.8</td><td>-0.096</td><td>-0.028</td><td>0.265</td><td>-0.206</td><td>-0.127</td><td>0.334</td><td>-0.063</td><td>-0.017</td><td>0.255</td></tr><tr><td>1.9</td><td>-0.193</td><td>-0.092</td><td>0.358</td><td>-0.221</td><td>-0.112</td><td>0.363</td><td>-0.061</td><td>-0.003</td><td>0.220</td></tr></tbody></table>

Note. The quoted colors correspond to the left bin edge. Simple Gaussian statistics do not fully capture the complexity of the responses—see Figure 18.

<table><caption>**Table C5**
Elements of the Classification (or Confusion) Matrix for Balrog Sources Binned by Injection Magnitude when Normalized by Percent, where the Measured Classification is Determined by EXTENDED_CLASS_SOF <= 1 for Stars and EXTENDED_CLASS_SOF > 1 for Galaxies</caption><thead><tr><th>True Mag</th><th>Star-&gt;Star<br>(TP; %)</th><th>Gal-&gt;Star<br>(FP; %)</th><th>Star-&gt;Gal<br>(FN; %)</th><th>Gal-&gt;Gal<br>(TN; %)</th></tr></thead><tbody><tr><td>18.50</td><td>99.6</td><td>1.6</td><td>0.4</td><td>98.4</td></tr><tr><td>18.75</td><td>99.6</td><td>2.9</td><td>0.4</td><td>97.1</td></tr><tr><td>19.00</td><td>99.4</td><td>2.9</td><td>0.6</td><td>97.1</td></tr><tr><td>19.25</td><td>99.3</td><td>2.6</td><td>0.7</td><td>97.4</td></tr><tr><td>19.50</td><td>99.2</td><td>2.8</td><td>0.8</td><td>97.2</td></tr><tr><td>19.75</td><td>99.1</td><td>2.3</td><td>0.9</td><td>97.7</td></tr><tr><td>20.00</td><td>98.7</td><td>1.9</td><td>1.3</td><td>98.1</td></tr><tr><td>20.25</td><td>98.6</td><td>1.8</td><td>1.4</td><td>98.2</td></tr><tr><td>20.50</td><td>98.2</td><td>1.8</td><td>1.8</td><td>98.2</td></tr><tr><td>20.75</td><td>97.8</td><td>1.9</td><td>2.2</td><td>98.1</td></tr><tr><td>21.00</td><td>97.3</td><td>1.8</td><td>2.7</td><td>98.2</td></tr><tr><td>21.25</td><td>96.7</td><td>1.7</td><td>3.3</td><td>98.3</td></tr><tr><td>21.50</td><td>95.9</td><td>2.2</td><td>4.1</td><td>97.8</td></tr><tr><td>21.75</td><td>95.1</td><td>2.0</td><td>4.9</td><td>98.0</td></tr><tr><td>22.00</td><td>93.4</td><td>2.3</td><td>6.6</td><td>97.7</td></tr><tr><td>22.25</td><td>90.8</td><td>3.2</td><td>9.2</td><td>96.8</td></tr><tr><td>22.50</td><td>86.4</td><td>4.1</td><td>13.6</td><td>95.9</td></tr><tr><td>22.75</td><td>79.5</td><td>5.2</td><td>20.5</td><td>94.8</td></tr><tr><td>23.00</td><td>70.3</td><td>6.7</td><td>29.7</td><td>93.3</td></tr><tr><td>23.25</td><td>58.2</td><td>8.3</td><td>41.8</td><td>91.7</td></tr><tr><td>23.50</td><td>46.4</td><td>10.1</td><td>53.6</td><td>89.9</td></tr><tr><td>23.75</td><td>37.5</td><td>12.4</td><td>62.5</td><td>87.6</td></tr><tr><td>24.00</td><td>30.9</td><td>14.5</td><td>69.1</td><td>85.5</td></tr><tr><td>24.25</td><td>25.9</td><td>15.0</td><td>74.1</td><td>85.0</td></tr></tbody></table>

Note. The second through fifth columns correspond to the true-positive (TP), false-positive (FP), false-negative (FN), and true-negative (TN) rates of Balrog stars, respectively. The very pure δ-stars sample is used to compute the TP and FN rates, while the noisier classifications of the DF y3-deep injections are used for the rest. The quoted magnitudes correspond to the left bin edge. See Figure 23.

ORCID iDs

S. Everett https://orcid.org/0000-0002-3745-2882

B. Yanny https://orcid.org/0000-0002-9541-2678

N. Kuropatkin https://orcid.org/0000-0003-2511-0946

E. M. Huff https://orcid.org/0000-0002-9378-3424

J. Myles https://orcid.org/0000-0001-6145-5859

J. Elvin-Poole https://orcid.org/0000-0001-5148-9203

G. M. Bernstein https://orcid.org/0000-0002-8613-8259

I. Sevilla-Noarbe https://orcid.org/0000-0002-1831-1953

E. Sheldon https://orcid.org/0000-0001-9194-0441

D. Gruen https://orcid.org/0000-0003-3270-7644

K. Eckert https://orcid.org/0000-0002-1407-4700

M. R. Becker https://orcid.org/0000-0001-7774-2246

H. T. Diehl https://orcid.org/0000-0002-8357-7467

D. L. Tucker https://orcid.org/0000-0001-7211-5729

E. Bertin https://orcid.org/0000-0002-3602-3664

T. Jeltema https://orcid.org/0000-0001-6089-0365

A. Drlica-Wagner https://orcid.org/0000-0001-8251-933X

R. A. Gruendl https://orcid.org/0000-0002-4588-6517

T. M. C. Abbott https://orcid.org/0000-0003-1587-3931

M. Aguena https://orcid.org/0000-0001-5679-6747

J. Annis https://orcid.org/0000-0002-0609-3987

J. Carretero https://orcid.org/0000-0002-3130-0204

F. J. Castander https://orcid.org/0000-0001-7316-4573

C. Conselice https://orcid.org/0000-0003-1949-7638

M. Costanzi https://orcid.org/0000-0001-8158-1449

J. DeRose https://orcid.org/0000-0002-0728-0960

P. Fosalba https://orcid.org/0000-0002-1510-5214

J. García-Bellido https://orcid.org/0000-0002-9370-8360

E. Gaztanaga https://orcid.org/0000-0001-9632-0815

D. W. Gerdes https://orcid.org/0000-0001-6942-2736

S. R. Hinton https://orcid.org/0000-0003-2071-9349

D. L. Hollowood https://orcid.org/0000-0002-9369-4157

D. Huterer https://orcid.org/0000-0001-6558-0112
S. Kent https://orcid.org/0000-0003-4207-7420

K. Kuehn https://orcid.org/0000-0003-0120-0808

J. L. Marshall https://orcid.org/0000-0003-0710-9474

P. Melchior https://orcid.org/0000-0002-8873-5065

F. Menanteau https://orcid.org/0000-0002-1372-2534

R. Miquel https://orcid.org/0000-0002-6610-4836

A. Palmese https://orcid.org/0000-0002-6011-0530

F. Paz-Chinchón https://orcid.org/0000-0003-1339-2683

A. K. Romer https://orcid.org/0000-0002-9328-879X

A. Roodman https://orcid.org/0000-0001-5326-3486

S. Serrano https://orcid.org/0000-0002-0211-2861

M. Soares-Santos https://orcid.org/0000-0001-6082-8529

G. Tarle https://orcid.org/0000-0003-1704-0781

J. Weller https://orcid.org/0000-0002-8282-2010

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