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Table 1
Photometric data of the three NB selected objects we studied.
| Instrument | Filter | Central wavelength (nm) | Obj1 | Obj2 | Obj3 |
|
|
|||||
| WIRCam | Ks | 2146 | >24.70 | >24.70 | >24.70 |
| WIRCam | H | 1631 | >24.70 | >24.70 | >24.70 |
| HAWK-I | J | 1258 | >26.53 | >26.53 | >26.53 |
| HAWK-I | NB1060 | 1062 | 24.3 ± 0.1 | 24.30 ± 0.06 | 24.52 ± 0.05 |
| Megacam | z ′ | 890 | >26.6 | 26.59 ± 0.40 | 26.43 ± 0.31 |
| Megacam | i ′ | 770 | 27.1 ± 0.2 | >27.43 | 27.02 ± 0.19 |
| Megacam | r ′ | 625 | 27.3 ± 0.2 | 27.41 ± 0.21 | >28.0 |
| Megacam | g′ | 486 | 27.3 ± 0.2 | 27.44 ± 0.19 | 27.89 ± 0.27 |
| Megacam | u⋆ | 378 | 27.1 ± 0.3 | >27.37 | >27.37 |
Notes. The significance of the limiting magnitudes is 3σ.
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