Table B.1
Counterparts of the extracted radio sources at different wavelengths.
| ID | Name | Known | Candidate | Radio-quiet | 2MASS | GLIMPSE | WISE | MIPSGAL | Hi-GAL | ATLASGAL | MAGPIS | MeerKAT | |||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| H II | H II | H II | 1.25–2.16 μm | 3.6 μm | 4.5 μm | 8.0 μm | 12 μm | 22 μm | 24 μm | 70 μm | 160 μm | 250 μm | 350 μm | 500 μm | 870 μm | 6 cm | 23.52 cm | ||
| 1 | G35S.632+0.063 | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓c | ✓ | ||||
| 2 | G358.917+0.072 | ✓c | ✓c | ✓ | |||||||||||||||
| 3 | G358.803-0.011 | ✓ | ✓c | ✓ | ✓ | ✓ | ✓ | ✓ | ✓* | ✓ | ✓ | ✓ | ✓c | ✓c | ✓ | ||||
| 4 | G35S.644-0.033 | ✓ | ✓c | ✓ | ✓ | ✓ | ✓ | ✓* | ✓ | ✓c | ✓c | ✓ | |||||||
| 5 | G358.599-0.060 | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓* | ✓ | ✓c | ✓c | ✓ | |||||||
| 6 | G358.683-0.116 | ✓ | ✓c | ✓ | ✓ | ✓ | ✓ | ✓* | ✓ | ✓ | ✓c | ✓c | ✓c | ✓ | |||||
| 7 | G35S.696+0.263 | ✓c | ✓c | ✓ | |||||||||||||||
| S | G358.784+0.060 | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓* | ✓ | ✓c | ✓ | ||||||||
| 9 | G35S.720+0.010 | ✓ | ✓c | ✓ | ✓ | ✓ | ✓ | ✓ | ✓* | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓c | ✓ | ||
| 10 | G358.719-0.125 | ✓ | ✓c | ✓c | ✓ | ✓ | ✓* | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓c | ✓ | ||||
| 11 | G358.592+0.046 | ✓c | ✓ | ||||||||||||||||
| 12 | G35S.S49+0.161 | ✓c | ✓ | ✓ | ✓c | ✓c | ✓ | ||||||||||||
| 13 | G35S.710+0.136 | ✓c | ✓ | ✓ | ✓c | ✓c | ✓ | ||||||||||||
| 14a | G35S.529+0.059 | ✓ | ✓c | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓c | ✓c | ✓ | ||||||
| 14b | G358.521+0.028 | ✓ | ✓ | ✓ | ✓ | ✓c | ✓ | ||||||||||||
| 14c | G35S.4S2+0.074 | ✓ | ✓c | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ||||||||||
| 15 | G358.551-0.029 | ✓ | ✓ | ✓ | ✓ | ✓ | ✓c | ✓ | |||||||||||
| 16 | G35S.651-0.077 | ✓ | ✓c | ✓ | ✓ | ✓ | ✓ | ✓* | ✓ | ✓ | |||||||||
| 17 | G358.844+0.026 | ✓ | ✓c | ✓ | ✓ | ✓ | ✓ | ✓ | ✓* | ✓ | ✓c | ✓c | ✓ | ||||||
| 18 | G358.881+0.056 | ✓ | ✓c | ✓ | ✓ | ✓ | ✓ | ✓ | ✓* | ✓ | ✓ | ✓ | ✓c | ✓ | ✓c | ✓ | |||
| 19 | G358.505+0.108 | ✓ | ✓ | ✓ | ✓ | ||||||||||||||
| 20 | G35S.S90+0.0S2 | ✓ | ✓c | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓c | ✓ | ✓ | ||||
| 21a | G358.689-0.076 | ✓ | ✓c | ✓ | ✓ | ✓ | ✓ | ✓ | ✓* | ✓ | ✓ | ||||||||
| 21b | G358.681-0.088 | ✓ | ✓ | ✓ | ✓ | ✓* | ✓ | ✓ | |||||||||||
| 22 | G358.612+0.178 | ✓ | ✓ | ✓ | ✓c | ✓c | ✓c | ✓ | |||||||||||
| 23 | G358.758+0.203 | ✓c | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓c | ✓c | ✓ | ||||||||
| 24 | G358.824+0.084 | ✓ | ✓c | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓c | ✓ | |||||||
| 25 | G358.753+0.053 | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ||||||||||
| 26 | G35S.7S9-0.020 | ✓c | ✓c | ✓c | ✓c | ✓ | ✓ | ✓ | ✓c | ✓ | |||||||||
| 27 | G358.614-0.034 | ✓c | ✓ | ✓ | ✓ | ||||||||||||||
| 28 | G358.823-0.118 | ✓c | ✓c | ✓ | ✓ | ✓c | ✓ | ||||||||||||
| 29 | G35S.S22+0.000 | ✓c | ✓ | ✓ | ✓ | ✓c | ✓c | ✓ | |||||||||||
| 30 | G358.773+0.031 | ✓ | ✓c | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ||||||||
| 31 | G358.595+0.101 | ✓ | ✓ | ✓ | ✓ | ✓ | ✓c | ✓ | |||||||||||
| 32 | G358.533-0.100 | ✓c | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | |||||||||||
| 33 | G358.466+0.064 | ✓ | ✓c | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓c | ✓ | |||||||
| 34 | G358.712+0.038 | ✓ | ✓c | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ||||||||
| 35 | G358.747-0.154 | ✓ | ✓c | ✓ | ✓ | ✓ | ✓ | ✓ | ✓c | ||||||||||
| 36 | G358.622+0.093 | ✓c | ✓c | ✓ | |||||||||||||||
| 37 | G358.905+0.029 | ✓ | ✓c | ✓c | ✓ | ||||||||||||||
| 38 | G358.557+0.243 | ✓c | ✓c | ✓ | ✓ | ||||||||||||||
| 39 | G358.510+0.178 | ✓c | ✓ | ✓ | ✓c | ✓ | ✓ | ✓ | |||||||||||
| 40 | G358.561-0.095 | ✓ | ✓c | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ||||||||
| 41 | G35S.714+0.054 | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓c | ✓ | |||||||||
| 42 | G358.631-0.122 | ✓c | ✓c | ✓c | ✓ | ||||||||||||||
| 43 | G358.804+0.037 | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ✓ | ||||||||||
| 44 | G35S.633+0.240 | ✓c | ✓ | ✓ | ✓c | ||||||||||||||
| 45 | G358.559-0.061 | ✓c | ✓c | ✓c | ✓ | ✓ | ✓c | ✓ | |||||||||||
| 46 | G35S.6SS+0.1S2 | ✓c | ✓c | ✓c | ✓c | ✓ | ✓ | ||||||||||||
Notes. The known, candidate and radio-quiet H II region columns list the cross-matches from the WISE H II catalog (V2.3; Anderson et al. 2014) with a tickmark (✓). The tickmarks in the remaining columns list the source with observed signature in the respective images. The superscript (*) represents the saturation in the MIPSGAL 24 μm image. The sources having counterparts in the respective catalogs for GLIMPSE 3.6, 4.5 and 8 μm, MIPSGAL 24 μm, and Hi-GAL 70–500 μm emission, given in Tab. B.2, but not displaying any clear visual signature in the images are represented with the superscript (c). The counterparts for 2MASS 1.25–2.16 μm and MAGPIS 6 cm are determined only from their respective catalogs provided in Tab. B.2, and are also marked with the superscript (c). The MeerKAT counterparts were visually identified from the ‘1.28 GHz MeerKAT GC mosaic’ (Heywood et al. 2022).
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