Table B.9
Sources with discarded association in our ATCA/VLA observations.
| Radio continuum emission | Maser emission | ||||||
|---|---|---|---|---|---|---|---|
| Source name | Position | Flux densitya | Frequency | Source name | Position | Flux densityb | Transition |
| RA, DEC (J2000) | (mJy) | (GHz) | RA, DEC (J2000) | (Jy) | |||
| RACS-DR1 J141249.8–69210 | 14:12:50.756 −69:21:03.56 | 48.6±0.7 | 2.1 | IRAS 14086–6907 | 14:12:50.393 −69:21:09.75 | 5.61±0.04 | OH 1612 MHz |
| IRAS 15559–5546 | 15:59:57.644 −55:55:33.24 | 69.3±1.8 | 2.1 | IRAS 15557–5546 | 15:59:41.667 −55:54:51.21 | 1.49±0.06 | OH 1612 MHz |
| IRAS 17385–2211 | 17:41:36.590 −22:13:03.90 | 0.68±0.09 | 2.1 | IRAS 17388–2203 | 17:41:48.979 −22:05:17.03 | 2.56±0.05 | OH 1612 MHz |
| <1.0 | 1.5 | 17:41:48.963 −22:05:15.27 | 2.53±0.03 | OH 1612 MHz | |||
| 17:41:36.610 −22:13:03.37 | 0.70±0.05 | 24 | <42 | H2O 22 GHz | |||
| GPSR 020.590+0.425 | 18:27:07.018 −10:46:08.70 | 20.2±1.0 | 2.1 | IRAS 18243–1048 | 18:27:08.273 −10:46:06.93 | 0.92±0.04 | OH 1612 MHz |
| NGC 6644 | 18:32:34.682 −25:07:44.15 | 13.0±0.3 | 2.1 | IRC–20491 | 18:32:07.675 −24:57:18.95 | 3.084±0.05 | OH 1612 MHz |
| 18:32:34.687 −25:07:44.27 | 79.2±1.6 | 1.5 | 18:32:07.675 −24:57:18.95 | 3.09±0.04 | OH 1612 MHz | ||
| 18:32:34.689 −25:07:44.18 | 78.0±0.4 | 24 | <42 | H2O 22 GHz | |||
| K 3-33 | 19:22:26.694 +10:41:23.19 | 13.0±0.3 | 2.1 | IRAS 19201+1040 | 19:22:29.168 +10:46:21.62 | 1.23±0.05 | OH 1612 MHz |
| 19:22:26.669 +10:41:21.06 | 10.7±0.5 | 1.5 | 19:22:29.172 +10:46:21.00 | 2.56±0.05 | OH 1612 MHz | ||
| 19:22:26.645 +10:41:20.30 | 15.34±0.08 | 24 | <36 | H2O 22 GHz | |||
Notes: a For sources in which radio continuum emission is not detected, we report the 3 σ upper limit to the intensity (in mJy beam−1). b For sources in which maser emission is not detected, we also report the 3 σ upper limit, using the noise level (in mJy beam−1), measured at the position and channel map with the VLSR of the reported OH maser from single-dish observations.
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