Table B.1
Magnitudes in the four Euclid bands.
| Archangel | AutoProf | |||||||
|---|---|---|---|---|---|---|---|---|
| Name | IE | YE | JE | HE | IE | YE | JE | HE |
| UGC02665 (spiral) | 13.92 | 13.12 | 12.97 | 12.79 | 13.92 | 13.12 | 12.97 | 12.79 |
| WISEAJ031917_76+413839_6 (elliptical) | 13.61 | 12.78 | 12.65 | 12.47 | 13.57 | 12.97 | 12.59 | 12.41 |
| EDwC-0120 (dwarf) | 18.88 | 18.35 | 18.26 | 18.23 | 18.85 | 17.97 | 17.52 | 17.81 |
Notes. Direct estimates of the uncertainties on magnitudes derived by Archangel and AutoProf are negligible, while the uncertainties derived by varying the sky background and fitting the growth curve are below 0.05 but for the dwarf galaxy. Magnitudes obtained with both software codes are very similar, if not equal, and differences are below a few percent. The difference in the NISP magnitudes for the dwarf galaxy can be explained by the different definitions of the radius, with the curves of growth being in very good agreement, as shown in Fig. B.3.
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