Table 2
Herschel observation setup parameters.
Clump | Line | RA | Dec | t | HPBW | Band | ν | Eup/k | ID | η mb | Date |
(h:m:s) | (°:′:′′) | (s) | (arcsec) | (GHz) | (K) | (yy/mm/dd) | |||||
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) |
|
|||||||||||
C1 | 8 → 7 | 18:42:47.29 | –4:04:06.1 | 265.5 | 23 | 3b | 921.79970 | 199 | 1342251119 | 0.628 | 12/09/18 |
C1 | 9 → 8 | 18:42:47.29 | –4:04:06.1 | 1332 | 20 | 4a | 1036.91239 | 249 | 1342254432 | 0.635 | 12/10/24 |
C1 | 10 → 9 | 18:42:47.29 | –4:04:06.1 | 1425.6 | 19 | 5a | 1151.98544 | 304 | 1342253926 | 0.590 | 12/10/26 |
F1 | 8 → 7 | 18:53:15.65 | 1:26:21.8 | 1110 | 23 | 3b | 921.79970 | 199 | 1342252136 | 0.628 | 12/10/03 |
F1 | 9 → 8 | 18:53:15.65 | 1:26:21.8 | 1332 | 20 | 4a | 1036.91239 | 249 | 1342254434 | 0.635 | 12/10/25 |
F1 | 10 → 9 | 18:53:15.65 | 1:26:21.8 | 1425.6 | 19 | 5a | 1151.98544 | 304 | 1342253937 | 0.590 | 12/10/26 |
F2 | 8 → 7 | 18:53:19.22 | 1:26:47.2 | 814 | 23 | 3b | 921.79970 | 199 | 1342244947 | 0.628 | 12/04/25 |
F2 | 9 → 8 | 18:53:19.22 | 1:26:47.2 | 1776 | 20 | 4a | 1036.91239 | 249 | 1342254433 | 0.635 | 12/10/25 |
F2 | 10 → 9 | 18:53:19.22 | 1:26:47.2 | 1425.6 | 19 | 5a | 1151.98544 | 304 | 1342253936 | 0.590 | 12/10/26 |
G2 | 8 → 7 | 18:56:49.67 | 1:23:15.4 | 265.5 | 23 | 3b | 921.79970 | 199 | 1342244946 | 0.628 | 12/04/25 |
G2 | 9 → 8 | 18:56:49.67 | 1:23:15.4 | 1332 | 20 | 4a | 1036.91239 | 249 | 1342254351 | 0.635 | 12/11/03 |
G2 | 10 → 9 | 18:56:49.67 | 1:23:15.4 | 1425.6 | 19 | 5a | 1151.98544 | 304 | 1342253938 | 0.590 | 12/11/03 |
Notes. Column 1 gives the name of the clump observed while Col. 2 gives the 12CO transition observed. Columns 3 and 4 are the right ascension and declination, respectively, of the map centres. The on source integration time of the observation is given in Col. 5. The average half power beam width of the H and V polarizations is given in Col. 6 and the Herschel frequency band of the observation is given in Col. 7. Columns 8 and 9, respectively, give the rest frequency and upper level energy, in units of kelvin, of the observed transition from the Spectral Line Atlas of Interstellar Molecules (SLAIM; Remijan et al. 2007). Columns 10 and 11 give the observation ID and the main beam conversion factor used. The main beam conversion factor used is the average of the appropriate values for the H and V polarizations based on the revised values of Jellema et al. (in prep.). Finally, Col. 12 gives the date the observation was conducted.
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