Table 5:
Fit of the magnitude uncertainty as a function of magnitude
deduced from the common areas. This
was used to compute uncertainties for individual galaxies: Uncertainty =
slope
magnitude + constant term.
Magnitude band |
validity domain |
slope |
constant term |
B |
[20,25.5] |
0.0340 |
-0.5933 |
V |
[20,24.5] |
0.0445 |
-0.8352 |
R |
[20,24] |
0.0420 |
-0.7410 |
I |
[20,23.5] |
0.0657 |
-1.1772 |
Source LaTeX |
All tables |
In the text