Table 1.
Continuum fluxes and integrated line intensities.
| Source | Continuum | Continuum | I[CI](2 − 1) | ICO(7 − 6) | I[CI](2 − 1) | ICO(7 − 6) | I[CI](2 − 1) | ICO(7 − 6) |
|---|---|---|---|---|---|---|---|---|
| frequency | flux | APEX | APEX | ALMA | ALMA | APEX | APEX | |
| (Narrow) | (Narrow) | (Broad) | (Broad) | |||||
| (GHz) | (mJy) | (Jy km s−1) | (Jy km s−1) | (Jy km s−1) | (Jy km s−1) | (Jy km s−1) | (Jy km s−1) | |
| SPT0103–45 | 208.93 | 25.52 ± 2.73 | 7.59 ± 2.34 | < 13.72 (3σ) | 15.29 ± 1.75 | 14.38 ± 1.43 | < 21.6 (3σ) | < 18.0 (3σ) |
| SPT2147–50 | 173.91 | 6.94 ± 0.84 | < 8.17 (3σ) | < 9.21 (3σ) | 4.94 ± 0.83 | 5.92 ± 0.90 | < 7.29 (3σ) | 8.95 ± 1.88 |
| SPT2357–51 | 190.99 | 8.18 ± 1.11 | < 9.34 (3σ) | 8.71 ± 2.14 | 3.63 ± 0.60 | 5.71 ± 0.80 | 5.88 ± 2.14 | 10.86 ± 2.42 |
Notes. Continuum fluxes are estimated from the continuum maps produced for the sources (Sect. 3.2). Line fluxes are estimated from the integrated intensity maps of the lines (Sect. 4.3). The uncertainties on these fluxes are the statistical uncertainties combined with a 10% absolute calibration uncertainty. APEX intensities are estimated by summing the fluxes for all the channels in a manually defined velocity range. The fourth and fifth columns are the fluxes estimated in a velocity window estimated from the APEX data (narrow window, Sect. 2.1), while the eighth and night columns correspond to the flux estimated using the same velocity range as in the ALMA spectra (broad window, Sect. 4.2). All the errors given are 1σ errorbars, except for the upper limits which are 3σ.
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