Table 3
UV to NIR photometry of the optical counterpart.
Band | Magnitude | Catalogue | Ref. | |
OGLE 9 | OGLE 74 | |||
|
||||
U | 14.018 ± 0.080 | 20.317 ± 0.175 | MCPS | 1 |
B | 15.016 ± 0.022 | 18.513 ± 0.061 | MCPS | 1 |
V | 14.945 ± 0.026 | 17.046 ± 0.035 | MCPS | 1 |
V | 15.106 ± 0.017 | 17.097 ± 0.011 | OGLE-III | 2 |
I | 14.894 ± 0.038 | 15.672 ± 0.186 | MCPS | 1 |
I | 14.906 ± 0.023 | 15.702 ± 0.007 | OGLE-III | 2 |
I | 14.783 ± 0.04 | – | DENIS | 3 |
J | 14.770 ± 0.039 | 14.637 ± 0.069 | 2MASS | 4 |
K | 14.354 ± 0.080 | 13.696 ± 0.054 | 2MASS | 4 |
|
||||
Band | OGLE 9 | Instrument | Ref. | |
|
||||
UVW1 | 14.94 ± 0.03 | Swift/UVOT | 5 | |
g ′ | 14.80 ± 0.05 | GROND | 5 | |
r ′ | 15.02 ± 0.04 | GROND | 5 | |
i ′ | 15.21 ± 0.04 | GROND | 5 | |
z ′ | 15.42 ± 0.04 | GROND | 5 | |
J | 15.72 ± 0.06 | GROND | 5 | |
H | 16.01 ± 0.07 | GROND | 5 | |
K | 16.41 ± 0.09 | GROND | 5 |
Notes.OGLE-III magnitudes are the average of 38 and 378 measurements in the V and I band, respectively. From Swift we give the UVW1 magnitude (in the AB photometric system), based on an average of six 200 s exposures taken on MJD 56 202.
Reference. (1) Zaritsky et al. (2004); (2) Udalski et al. (2008a); (3) DENIS Consortium (2005); (4) Skrutskie et al. (2006); (5) this work.
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