Table 5.
Likely matches to the UGS.
| 3FGL name | LDR1 name | Separation (°) | MQC | z | α | SMHz (mJy) |
|---|---|---|---|---|---|---|
| 3FGL J1051.0+5332 | ILTJ104931.19+533623.6 | 0.235 | Yes | 1.2582 | – | 1.17 ± 0.14 |
| 3FGL J1051.0+5332 | ILTJ105106.97+533143.0 | 0.023 | Yes | 1.1291 | – | 0.85 ± 0.19 |
| 3FGL J1051.0+5332 | ILTJ105238.00+533738.3 | 0.247 | Yes | 0.4025 | −0.34 | 15.23 ± 0.25 |
| 3FGL J1103.3+5239 | ILTJ110327.25+523425.1 | 0.09 | No | 0.3716 | – | 1.06 ± 0.11 |
Notes. Only one source was detected in another survey (NVSS) which we used to calculate α. There is no uncertainty listed as the fit is degenerate. We also list whether or not the LDR1 sources can be found in the Million Quasar Catalogue (MQC; Flesch 2017), which is a compendium of quasars and high-confidence quasar candidates.
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