Passband | Ba | Bb |
V | 24.12 ![]() |
![]() ![]() |
R | 20.65 ![]() |
22.35 ![]() |
I | 17.15 ![]() |
18.91 ![]() |
z | 15.07 ![]() |
16.53 ![]() |
J | 12.20 ![]() |
12.96 ![]() |
H | 11.60 ![]() |
13.40 ![]() |
K | 11.42 ![]() |
13.64 ![]() |
L' | 9.71 ![]() |
11.33 ![]() |
M' | 10.67 ![]() |
11.04 ![]() |
The optical magnitudes are in the FORS2 system as described in Appendix C, and the near-IR magnitudes have been transformed into the MKO
filters
via synthetic photometry. The uncertainties for both objects are
dominated by the uncertainties on the measured flux ratio and the
standard star magnitudes. Absolute magnitudes may be derived using the
distance
modulus of -2.205.
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