Table 2
Observation log for the H
O pointed observations and H2O 987 GHz maps.
| Source | Species | ObsID (a) |  |
rms (c) |
|---|---|---|---|---|
| (s) | (mK) | |||
| IRAS 05358 | H O |
206124, 206126 | 3566 | 20 |
| H2O | 204508 | 5.86 | 481 | |
| IRAS 16272 | H O |
214417, 214419 | 3455 | 20 |
| H2O | 203166 | 5.86 | 473 | |
| NGC 6334I(N) | H O |
206383 | 2965 | 22 |
| H2O | 204523 | 5.86 | 481 | |
| W43–MM1 | H O |
191670, 207372 | 3566 | 20 |
| H2O | 215899 | 5.86 | 524 | |
| DR21(OH) | H O |
194794, 197974 | 3566 | 20 |
| H2O | 210042 | 7.86 | 396 | |
| W3IRS5 | H O |
191658, 201591 | 3566 | 20 |
| H2O | 203160 | 5.86 | 498 | |
| IRAS 18089 | H O |
229882, 229883 | 3455 | 20 |
| H2O | 218210 | 5.86 | 557 | |
| W33A | H O |
191638, 208086 | 3566 | 20 |
| H2O | 215902 | 5.86 | 465 | |
| IRAS 18151 | H O |
229880, 229881 | 3455 | 20 |
| H2O | 218212 | 5.86 | 659 | |
| AFGL 2591 | H O |
194795, 197973 | 3566 | 20 |
| H2O | 210038 | 5.86 | 446 | |
| G327 | H O |
214422, 214423, 214425, 214426 | 3428 | 21 |
| H2O | 203169 | 5.86 | 490 | |
| NGC 6334I | H O |
206385 | 2965 | 22 |
| H2O | 204522 | 5.86 | 486 | |
| G29.96 | H O |
191668, 191669, 229875, 229876 | 3700 | 20 |
| H2O | 207655 | 5.86 | 475 | |
| G31.41 | H O |
191671, 191672, 229873, 229874 | 3700 | 20 |
| H2O | 207654 | 5.86 | 477 | |
| G5.89 | H O |
229888, 229889, 229890, 229891 | 3148 | 21 |
| H2O | 218201 | 5.86 | 575 | |
| G10.47 | H O |
229884, 229885, 229886, 229887 | 3148 | 21 |
| H2 O | 218208 | 5.86 | 476 | |
| G34.26 | H O |
191673, 191674, 229871, 229872 | 3700 | 20 |
| H2 O | 207652 | 5.86 | 493 | |
| W51 | H O |
194801, 194802, 207384, 207385 | 3420 | 20 |
| H2 O | 207651 | 5.86 | 485 | |
| NGC 7538IRS1 | H O |
191663, 191664, 197976 | 3569 | 20 |
| H2 O | 203161 | 5.86 | 479 | |
Notes. (a) The leading 1342 has been omitted. (b)For pointed observations, the integration time is for the total spectra, i.e. all ObsIDs added. For maps, the integration time is per observed position. (c) The rms is the noise in δν = 1.1 MHz. For pointed observations, the integration time is for the total spectra, i.e. all ObsIDs added.
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