Table 4: Typical values of the different considered error sources. Phot.: photonic noise; Flux: flux calibration; Wave.: wavelength calibration; Dichr.: typical error in the subtraction of the dichroic pattern (this error is only added in the measurements of Run 2). Res.: residual errors, based on repeated observations of 10 galaxies.
Index Phot. Flux Wave. Dichr. Res.
        (Run 2)  

D4000
0.006 0.088 0.000 0.001 0.000 Å
H$\delta_A$ 0.156 0.038 0.005 0.053 0.000 Å
H$\delta_F$ 0.104 0.009 0.009 0.021 0.000 Å
CN1 0.004 0.002 0.000 0.003 0.001 mag
CN2 0.005 0.003 0.000 0.003 0.010 mag
Ca4227 0.072 0.002 0.006 0.023 0.000 Å
G4300 0.121 0.014 0.013 0.138 0.074 Å
H$\gamma_A$ 0.143 0.033 0.002 0.121 0.302 Å
H$\gamma_F$ 0.087 0.012 0.003 0.062 0.072 Å
Fe4383 0.167 0.045 0.019 0.114 0.161 Å
Ca4455 0.086 0.004 0.024 0.024 0.000 Å
Fe4531 0.127 0.015 0.012 0.026 0.000 Å
C4668 0.186 0.171 0.010 0.012 0.054 Å
H$\beta $ 0.078 0.010 0.007 0.003 0.029 Å
Fe5015 0.167 0.081 0.022 0.025 0.115 Å
Mgb 0.087 0.035 0.006 0.108 0.029 Å
Fe5270         0.050 Å
Fe5335         0.000 Å


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