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Table 2.
List of five NIR sources that could be extragalactic sources associated with UGS.
| 4FGL | ID | Z | Y | J | H | Ks | VVV ID | Sep. |
|---|---|---|---|---|---|---|---|---|
| J1745.6-3626 | RS17 | 19.140 ± 0.265 | 18.606 ± 0.234 | 18.091 ± 0.224 | 17.351 ± 0.205 | 16.793 ± 0.134 | VVV-J174555.13-362331.2 | 1.02″ |
| J1814.7-3420 | RS23 | 19.158 ± 0.134 | 18.768 ± 0.134 | 17.984 ± 0.071 | 17.174 ± 0.076 | 16.400 ± 0.034 | VVV-J181446.75-342341.3 | 0.63″ |
| J1816.4-2727 | RS24 | 17.795 ± 0.083 | 17.320 ± 0.075 | 16.532 ± 0.050 | 15.747 ± 0.045 | 15.160 ± 0.032 | VVV-J181628.80-272603.1 | 0.36″ |
| J1817.2-3035 | RS25 | 18.198 ± 0.099 | 17.730 ± 0.083 | 17.040 ± 0.058 | 16.232 ± 0.050 | 15.515 ± 0.031 | VVV-J181720.40-303300.0 | 0.44″ |
| J1828.2-3252 | RS33 | 16.575 ± 0.010 | 16.166 ± 0.011 | 15.501 ± 0.007 | 14.756 ± 0.008 | 14.274 ± 0.005 | VVV-J182817.04-325521.0 | 0.92″ |
Notes. The columns, from left to right, are: ID of UGS from 4FGL catalog; number identification for RS; the means of the Z, Y, J, H and Ks magnitudes; VVV identifications of NIR; separation between NIR and RS (expressed in arcsec).
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