Table 4
Comparison of the sky model and the Walker (1987) magnitudes with the Patat (2008) FORS 1 data.
| Filter | All | No Moon | ||||||||||||||
| N | ⟨Δm⟩ | σ Δm | σ obs | ⟨Δmw⟩ | σ Δm,w | N | ⟨Δm⟩ | σ Δm | σ obs | ⟨Δmw⟩ | σ Δm,w | |||||
|
|
||||||||||||||||
| U | 303 | + 0.053 | 0.230 | 0.521 | −0.113 | 0.725 | 239 | + 0.042 | 0.213 | 0.214 | −0.059 | 0.703 | ||||
| B | 303 | + 0.046 | 0.205 | 0.561 | + 0.269 | 0.430 | 239 | + 0.048 | 0.174 | 0.182 | + 0.196 | 0.407 | ||||
| V | 979 | + 0.000 | 0.192 | 0.563 | + 0.356 | 0.409 | 727 | + 0.006 | 0.175 | 0.255 | + 0.244 | 0.322 | ||||
| R | 1046 | + 0.009 | 0.199 | 0.447 | + 0.169 | 0.365 | 762 | −0.009 | 0.177 | 0.260 | + 0.083 | 0.287 | ||||
| I | 839 | −0.003 | 0.238 | 0.365 | + 0.413 | 0.326 | 615 | −0.040 | 0.208 | 0.287 | + 0.365 | 0.294 | ||||
Notes. Mean values ⟨Δm⟩ and standard deviations σΔm for magnitude differences between the model and observed data (Δm = mmodel − mobs) and standard deviations of the magnitudes of the observed data σobs are shown. Moreover, mean values ⟨Δmw⟩ and standard deviations σΔm,w for magnitude differences between the Moon phase related data of Walker and the Patat data are displayed. Results are listed for the full and dark-time samples. The number of spectra involved is indicated by N.
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