Table A.2.
Main properties of the telescopes used for the collected 12CO data.
| Telescope (1) | 12CO line | θbeam(2) | Units | Jy K−1 |
|---|---|---|---|---|
| [″] | [K, Jy, M⊙] | |||
| Single-dish | ||||
| BELL | (1–0) | 100 |  |
108 |
| FCRAO | (1–0) | 45 |  |
42 |
| IRAM-30 m | (1–0) | 22 |  |
4.8 |
| IRAM-30 m | (2–1) | 11 |  |
5.3 |
| JCMT | (2–1) | 22 |  |
27 |
| JCMT | (3–2) | 14.5 |  |
33 |
| NRAO-12 m | (1–0) | 55 |  |
35 |
| OSO | (1–0) | 34 |  |
12 |
| SEST | (1–0) | 44 |  |
27 |
| SEST | (2–1) | 24 |  |
41 |
| Interferometer | ||||
| NMA | (1–0) | – | S(3) | – |
| CARMA | (1–0) | – | M(H2) (4) | – |
| SMA | (1–0) | – | M(H2) (4) | – |
Notes.
BELL is the Bell 7 m telescope (Chu et al. 1978), FCRAO the 14 m Five College Radio Astronomical Observatory, IRAM-30 m the 30 m antenna of the Institut de Radioastronomie Millimétrique, NRAO-12 m the 12 m National Radio Astronomy Observatory, OSO the 25 m Onsala Space Observatory, the Swedish National Facility for Radio Astronomy, SEST the 15 m Swedish-ESO Submillimetre Telescope, JCMT the 15 m James Clerk Maxwell Telescope, NMA is the Nobeyama Millimeter Array, an interferometer of six 10 m antennas, CARMA, Combined Array for Research in Millimeter-wave Astronomy, an interferometer of six 10.4 m, nine 6.1 m, and eight 3.5 m antennas, SMA, Submillimeter Array, an interferometer of eight 6 m antennas.
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