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Table 7
Literature-searched sources at the position of GMRT sources with spectral index information.
| ID | Dist. | Nearest source name | Nearest source type | Comments |
|---|---|---|---|---|
| I03 | 9.1″ | 2MASS J08072621–4721354 | YSO candidate | |
| I08 | 2.8″ | 2MASS J08080880–4732335 | YSO candidate | |
| 13″ | 2MASS J08080942–4732249 | YSO candidate | ||
| I09 | 18.8″ | 2MASS J08082235−4710594 | YSO | Fermi excess |
| I23 | 1.9″ | WR 11 | WR star | Fermi excess |
| I26 | 7.3″ | MOST 0808-471 | Radio source | Fermi excess |
| 14.1″ | 2MASS J08094219-4719526 | Pre-main-sequence star | ||
| I36 | 7.2″ | IRAS 08084–4656 | IR point source | Fermi excess |
| I49 | 10.3″ | 2MASS J08111607–4711036 | YSO candidate |
Notes. ID: same as in Table 5; Dist: distance between the Simbad source and the detected source at the 325 MHz image; “Fermi excess” means that the 325 MHz source lays within the Fermi excess presented by Pshirkov (2016).
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