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Table 4.
Continuum flux densities and line upper limits based on IRAM-30 m for the associated (top) and then intervening systems (bottom).
| Target | νobs | Scont | Line | σ |
|---|---|---|---|---|
| (GHz) | (mJy) | (mJy) | ||
| B0003+38A | 93.808 | 90 | CO(1–0) | 7 |
| UM305 | 97.232 | 120 | CO(2–1) | 12 |
| 112.846 | 100 | HCO+(3–2) | 15 | |
| 4C-02.08 | 91.059 | 20 | HCO+(2–1) | 4.5 |
| J0229+0044 | 104.008 | 10 | CO(2–1) | 2.5 |
| J0229+0053 | 106.582 | 5 | CO(2–1) | 3.5 |
| B2 1045+35A | 96.570 | 45 | HCO+(2–1) | 3.5 |
| 124.811 | 30 | CO(2–1) | 6 | |
| 4C+32.44 | 84.263 | 240 | CO(1–0) | 9 |
| J1540−1453 | 74.035 | 25 | CO(2–1) | 7 |
| J1648+2224 | 126.440 | 175 | CO(2–1) | 5 |
| B2-2050+36 | 85.096 | 80 | CO(1–0) | 2.5 |
| 0738+313 | 94.389 | 370 | CO(1–0) | 3.5 |
| SBS0804+499 | 95.765 | 440 | CO(2–1) | 12 |
| 0827+243 | 151.196 | 610 | CO(2–1) | 5 |
| J0921+6215 | 109.592 | 850 | CO(2–1) | 7 |
| 0952+179 | 93.126 | 200 | CO(1–0) (a) | 3.5 |
| B3 1241+410 | 113.329 | 40 | CO(1–0) | 10 |
| HB1331+170 | 83.033 | 100 | CO(2–1) | 2.5 |
| 3C336 | 107.725 | 25 | HCO+(2–1) | 5 |
| 139.227 | 15 | CO(2–1) | 3.5 | |
| J1639+1127 | 106.823 | 340 | CO(1–0) | 10 |
| PKS2029+121 | 84.293 | 900 | HCO+(2–1) | 4 |
| 163.409 | 505 | CO(3–2) | 5 | |
| HB2355−106 | 106.090 | 490 | CO(2–1) | 4.5 |
Notes. The spectral rms (σ) is based on 20 km s−1 channels.
(a)
CO(4–3) detected by ALMA at zem (Audibert et al. 2022).
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