Table A.1
SiO lines used in this work.
| Transition | Rest Frequency | Eup | Telescope | Integrated Intensity [Jy km s−1 for ALMA and ACA; K km s−1 for others] | ||||
|---|---|---|---|---|---|---|---|---|
| [GHz] | [K] | |||||||
| 15194–5115 | 15082–4808 | 07454–7112 | AFGL 3068 | IRC +10 216 | ||||
| 1 − 0 | 43.423853 | 2.08 | Yebes | − | − | − | − | 15.4(b) |
| 2 − 1 | 86.846985 | 6.25 | ALMA | 96.1 | 35.1 | 15.8 | − | 422.5(c) |
| IRAM | − | − | − | − | 65.2(d) | |||
| 3 − 2 | 130.268683 | 12.50 | IRAM | − | − | − | − | 139.4(d) |
| 4 − 3 | 173.688238 | 20.84 | APEX | 12.4 | 1.2 | 2.4 | 0.9 | 62.1 |
| IRAM | − | − | − | − | 226.4(d) | |||
| 5 − 4 | 217.104919 | 31.26 | APEX | 15.2 | 1.2 | 3.6 | 0.9 | 75.4 |
| IRAM | − | − | − | − | 248.2(d) | |||
| ACA | − | − | 97.5(a) | 23.1(a) | − | |||
| 6–5 | 260.518009 | 43.76 | APEX | 13.6 | 1.2 | 4.2 | 0.9 | 89.9 |
| IRAM | − | − | − | − | 281.4(d) | |||
| 7 − 6 | 303.926812 | 58.35 | APEX | 13.8 | − | − | − | − |
| IRAM | − | − | − | − | 349.9(d) | |||
| 8 − 7 | 347.330581 | 75.02 | APEX | 14.4 | − | − | − | − |
| IRAM | − | − | − | − | 380.6(d) | |||
| 12 − 11 | 520.881187 | 162.52 | HIFI | 1.4 | − | − | − | − |
| 13 − 12 | 564.249098 | 189.60 | HIFI | 1.3 | − | − | − | − |
| 14 − 13 | 607.607719 | 218.76 | HIFI | 1.3 | − | − | − | − |
| 15 − 14 | 650.956290 | 250.00 | HIFI | 1.2 | − | − | − | − |
| 16 − 15 | 694.294114 | 283.32 | HIFI | 0.9 | − | − | − | − |
| 18 − 17 | 780.934648 | 356.20 | HIFI | 0.5 | − | − | − | − |
| 19 − 18 | 824.235900 | 395.75 | HIFI | 0.4 | − | − | − | − |
| 20 − 19 | 867.523546 | 437.39 | HIFI | 0.4 | − | − | − | − |
| 21 − 20 | 910.796851 | 481.10 | HIFI | 0.8 | − | − | − | − |
| 22 − 21 | 954.055103 | 526.89 | HIFI | 0.6 | − | − | − | − |
Notes. The ALMA and APEX lines reported for IRAS 15194–5115, IRAS 15082–4808, and IRAS 07454–7112 are from Paper I, unless otherwise specified. All HIFI lines listed are from our Herschel/HIFI spectral survey of IRAS 15194–5115 (see Paper I). For the ALMA (and ACA) lines, the integrated intensity values reported are in units of Jy km s−1 and are calculated using spectra extracted from apertures large enough to encompass all detected line emission. For all other SD observations (APEX, HIFI, IRAM, Yebes), the integrated intensities are given in units of K km s−1, in the main beam (TMB) temperature scale. The relevant beam size ranges and main beam efficiencies for the SD telescopes are described in Paper II, and the individual beam sizes at each transition frequency are indicated in Fig. 2 and the relevant figures in Appendix B, alongside the corresponding line spectra. (a) The DEATHSTAR ACA survey (Ramstedt et al. 2020; Andriantsaralaza et al. 2021); (b) Massalkhi et al. (2024); (c) Velilla-Prieto et al. (2019); (d) Agúndez et al. (2012).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.