Table A.1
Onsala 20 m telescope non-detections.
| Source | αJ2000 | δJ2000 | υLSR | Line | rms (*) |
|---|---|---|---|---|---|
| [kms−1] | [GHz] | [mK] | |||
| Orion | 05:35:16.96 | −05:22:02.7 | +9.7 | 68 | 40 |
| KL/S (1) | 69 | 33 | |||
| Orion | 05:35:14.28 | −05:22:27.5 | +9.0 | 70 | 24 |
| KL/S (2) | 68 | 53 | |||
| 69 | 48 | ||||
| Orion | 05:35:14.28 | −05:23:16.5 | +9.0 | 70 | 23 |
| KL/S (3) | 68 | 55 | |||
| 69 | 43 | ||||
| Orion | 05:35:16.46 | −05:23:22.7 | +9.0 | 70 | 27 |
| KL/S (4) | 68 | 61 | |||
| 69 | 37 | ||||
| Orion | 05:35:13.10 | −05:23:56.0 | +9.0 | 70 | 17 |
| KL/S (5) | 68 | 40 | |||
| 69 | 30 | ||||
| Orion | 05:35:24.96 | −05:22:32.7 | +9.0 | 68 | 30 |
| KL/S (6) | 69 | 25 | |||
| Orion | 05:35:25.30 | −05:24:34.0 | +11.0 | 70 | 17 |
| Bar (1) | 68 | 34 | |||
| 69 | 25 | ||||
| Orion | 05:35:22.80 | −05:25:01.0 | +11.0 | 68 | 55 |
| Bar (2) | 69 | 38 | |||
| Orion | 05:35:25.40 | −05:25:25.0 | +11.0 | 70 | 18 |
| Bar (3) | 68 | 41 | |||
| 69 | 30 | ||||
| Orion | 05:35:23.10 | −05:24:35.0 | +11.0 | 70 | 23 |
| Bar (4) | 68 | 47 | |||
| 69 | 41 | ||||
| Orion | 05:35:20.81 | −05:25:17.1 | +11.0 | 68 | 38 |
| Bar (5) | 69 | 28 | |||
| W51 E | 19:23:44.00 | 14:30:30.00 | +55.3 | 68 | 21. |
| 69 | 18 | ||||
| W51 M | 19:23:42.00 | 14:30:36.00 | +58.4 | 68 | 24 |
| 69 | 21 | ||||
| W51 N | 19:23:40.00 | 14:31:10.00 | +60.0 | 68 | 15 |
| 69 | 12 | ||||
| W49 N | 19:10:13.55 | 09:06:14.70 | +8.8 | 68 | 26 |
| 69 | 21 | ||||
| W43 | 18:47:36.89 | −01:55:30.20 | +91.1 | 68 | 26 |
| 69 | 19 | ||||
| DR21 | 20:39:02.00 | 42:19:42.00 | −2.5 | 68 | 11 |
| 69 | 7 | ||||
| W75 N | 20:38:36.45 | 42:37:35.10 | +7.5 | 68 | 9 |
| 69 | 8 | ||||
| S140 | 22:19:11.53 | 63:17:46.90 | −12.3 | 68 | 34 |
| 69 | 25 | ||||
| W3(OH) | 02:27:04.10 | 61:52:22.00 | −46.0 | 70 | 7 |
| 68 | 13 | ||||
| 69 | 8 | ||||
| S233 | 05:35:51.19 | 35:44:12.90 | −17.5 | 70 | 10 |
| 68 | 17 | ||||
| 69 | 15 | ||||
| S235 | 05:40:53.30 | 35:41:49.00 | −57.0 | 70 | 19 |
| 68 | 37 | ||||
| 69 | 30 | ||||
| CRL618 | 04:42:53.62 | 36:06:53.30 | −26.0 | 70 | 60 |
| 68 | 100 | ||||
| 69 | 80 | ||||
| CRL2688 | 21:02:18.27 | 36:41:37.00 | −32.0 | 70 | 12 |
| 68 | 20 | ||||
| 69 | 18 | ||||
| NGC 7023 | 21:01:36.90 | 68:09:48.00 | 2.5 | 70 | 12 |
| 68 | 24 | ||||
| 69 | 22 | ||||
| NGC 7027 | 21:07:01.75 | 42:14:10.00 | 8.9 | 70 | 6 |
| 68 | 11 | ||||
| 69 | 9 | ||||
| NGC 7538 | 23:13:37.20 | 61:30:00.00 | −64.9 | 70 | 19 |
| 68 | 38 | ||||
| 69 | 28 | ||||
| Cas A | 23:23:24.90 | 58:50:03.30 | −2600.0 | 70 | 8 |
| 68 | 15 | ||||
| 69 | 12 | ||||
| IC 443 | 06:18:02.70 | 22:39:03.00 | −4.4 | 70 | 10 |
| 68 | 16 | ||||
| 69 | 14 |
Notes. Columns are: (left to right) source name, J2000 coordinates of observed position, assumed LSR velocity, line ID, and 1σ rms noise level. (*)On the Tmb scale the rms noise is quoted for a spectral resolution of 0.97 km s−1. All the sources are SFRs, except for NGC 7027 which is a planetary nebula, CRL618 and CRL2688, which are proto-planetary nebulae and Cas A and IC 443, which are supernova remnants. NGC7023 is a reflection nebula with a PDR.
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