Table B.10
Sources with undetected continuum and/or maser emission in our ATCA/VLA observations.
| Target name | Date | Continuuma | Maserb | Telescope | Associationc | |
|---|---|---|---|---|---|---|
| Frequency | Flux density | Flux density | ||||
| (GHz) | (mJy) | (mJy) | ||||
| IRAS 14079–6402 | 2021/10/19 | 2.1 | 1.81±0.16 | <39 | ATCA | UM |
| IRAS 16280–4008 | 2021/10/19 | 2.1 | 615.3±1.5 | <87 | ATCA | UM |
| IRAS 17180–2708 | 2021/10/20 | 2.1 | 265.0±0.3 | <177 | ATCA | UM |
| 2021/04/03 | 1.5 | 268.6±1.8 | <117 | VLA | UM | |
| 2021/04/01 | 24 | 174.9±1.6 | <27 | VLA | UM | |
| IRAS 17221–3038 | 2021/10/20 | 2.1 | 8.60±0.13 | <114 | ATCA | UM |
| IRAS 17253–2824 | 2021/10/20 | 2.1 | <0.19 | 171±20 | ATCA | UC |
| 2021/04/03 | 1.5 | <2.0 | 224±14 | VLA | UC | |
| 2021/04/01 | 24 | <0.04 | <20.1 | VLA | UC, UM | |
| IRAS 17374–2700 | 2021/10/20 | 2.1 | <0.18 | <99 | ATCA | UC, UM |
| 2021/04/03 | 1.5 | <1.12 | <72 | VLA | UC, UM | |
| 2021/04/01 | 24 | <0.04 | <24 | VLA | UC, UM | |
| IRAS 17403–2107 | 2021/10/20 | 2.1 | 11.26±0.16 | <120 | ATCA | UM |
| 2021/04/03 | 1.5 | 11.8±0.5 | <114 | VLA | UM | |
| 2021/04/01 | 24 | 7.79±0.09 | <33 | VLA | UM | |
| IRAS 18271–1014 | 2021/10/19 | 2.1 | 1.5±0.4 | <33 | ATCA | UM |
| 2021/04/03 | 1.5 | <3 | <60 | VLA | UM | |
| 2021/04/01 | 24 | 1.95±0.09 | <18 | VLA | UM | |
| OH 25.646–0.003d | 2021/03/25 | 24 | <0.08 | <36 | VLA | UC, UM |
| IRAS 18551+0159 | 2021/04/03 | 1.5 | 143±5 | <210 | VLA | UM |
| 2021/03/25 | 24 | 189.6±0.4 | <42 | VLA | UM | |
| IRAS 19123+1139 | 2021/10/19 | 2.1 | 29.5±1.0 | <87 | ATCA | UM |
| 2021/03/25 | 1.5 | 33±3 | <237 | VLA | UM | |
| 2021/03/25 | 24 | 17.09±0.11 | <36 | VLA | UM | |
| IRAS 19127+1717 | 2021/10/19 | 2.1 | 0.79±0.16 | <60 | ATCA | UM |
| 2021/03/25 | 1.5 | 2.2±0.4 | <90 | VLA | UM | |
| 2021/03/25 | 24 | 5.94±0.05 | <33 | VLA | UM | |
| IRAS 19508+2659 | 2021/03/25 | 24 | <0.06 | 565±11 | VLA | UC |
| IRAS 20266+3856 | 2021/04/03 | 1.5 | <4 | 1336±180 | VLA | UC |
| 2021/03/25 | 24 | <0.06 | <45 | VLA | UC, UM | |
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. c UC: undetected continuum emission. UM: undetected maser emission. d This object is a new OHPN candidate, but we have included it in this table because we did not detect any H2O maser nor radio continuum emission in our VLA observations (see Appendix C.3.6).
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