Table 1
Overview of Herschel/HIFI observations of AFGL2591 used in this work.
| Band | Observing date | Herschel obsid | Freq. rangea | tobsb | rms noisec | Tsysd | HPBWe | ηmbf | |||
| (yyyy-mm-dd) | (GHz) | (s) | (mK) | (K) | (′′) | (%) | |||||
|
|
|||||||||||
| 1a | 2010-04-11 | 1 342 194 483 | 483–558 | 4592 | 30 | 74
|
44–38 | 75.5 | |||
| 1b | 2010-04-12 | 1 342 194 528 | 555–636 | 4643 | 29 | 87
|
38–33 | 75.3 | |||
| 2a | 2010-10-28 | 1 342 207 599 | 631–722 | 9833 | 26 | 142
|
34–29 | 75.1 | |||
| 2b | 2010-04-12 | 1 342 194 573 | 717–800 | 6407 | 67 | 188
|
30–27 | 74.9 | |||
| 3a | 2010-10-28 | 1 342 207 622 | 800–859 | 4893 | 39 | 200
|
27–25 | 74.7 | |||
| 3b | 2010-04-13 | 1 342 194 699 | 858–960 | 8578 | 67 | 205
|
25–22 | 74.4 | |||
| 4a | 2010-05-16 | 1 342 196 594 | 950–1060 | 9137 | 157 | 356
|
22–20 | 74.1 | |||
| 4b | 2010-05-11 | 1 342 196 428 | 1051–1120 | 6300 | 144 | 339
|
20–19 | 73.8 | |||
| 5a | 2010-05-12 | 1 342 196 510 | 1110–1240 | 11 931 | 147 | 913
|
19–17 | 63.7 | |||
| 5b | 2011-05-11 | 1 342 220 520 | ~1267 | 1380 | 149 | 1246 ±126 | 17 | 63.4 | |||
| 6a | 2011-04-21 | 1 342 219 224 | ~1497 | 1440 | 117 | 1507 ±143 | 14 | 71.8 | |||
| 6b | 2010-12-02 | 1 342 210 726 | ~1612 | 1392 | 106 | 1366 ±104 | 13 | 71.1 | |||
| 7a | 2010-12-04 | 1 342 210 803 | ~1727 | 1575 | 92 | 1300 ±43 | 12 | 70.5 | |||
| 7b | 2011-05-11 | 1 342 220 471 | ~1841 | 1711 | 92 | 1201 ±5 | 12 | 69.7 | |||
Notes.
Observations from bands 1a to 5a are spectral scans, those in bands 5b to 7b are single frequency settings spanning ~4 GHz.
Double sideband system temperature. For spectral scans (1a–5a): median of the individual datasets, with superscripts and subscripts denoting the deviations to the 90th and 10th percentiles, respectively. For pointed frequency settings (5b−7b): average of the values for the H- and V-datasets, with superscripts denoting the deviation to lowest and highest value.
Half-power beam width at the relevant frequency, calculated following Roelfsema et al. (2012). The two values for each spectral scan indicate the HPBW at the lower and upper edge of the band.
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