Table 4.
Inferred quantities from the observed line and continuum luminosities.
Target | MH2, dust | MH2, CO | MH2, [CII] | MH2, [CI] | log [C II]/[C I] | log [C II]/CO(7–6) | log [C I]/CO(7–6) |
---|---|---|---|---|---|---|---|
[1010 M⊙] | [1010 M⊙] | [1010 M⊙] | [1010 M⊙] | ||||
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
PJ036+03 |
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J0338+0021 |
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PJ159–02 |
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< 4.9 | > 1.252 |
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< − 0.237 |
J1048–0109 |
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J1104+2134 |
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J1319+0950 |
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J2054–0005 |
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< 7.8 | > 1.253 |
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< 0.046 |
J2219+0102 |
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PJ338+29 |
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< 4.6 | > 1.479 |
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< − 0.216 |
PJ359–06 |
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< 4.7 | > 1.575 |
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< − 0.181 |
Stack(a) |
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Notes. (1) Target name. (2–5) Molecular gas mass estimates from dust continuum (MH2, dust), CO (MH2, CO), [C I] (MH2, [CI]), and [C II] (MH2, [CII]), derived as described in the text. (6–8) Observed line luminosity ratios.
For the line ratios of the stacked spectrum, we adopt the average value L[CII] = 2.5 × 109 L⊙ based on the median value of the literature measurements in Table 1.
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