Table 6
Mean and median values.
| Sample | ⟨ log(MH2) ⟩ |
|
|
|
|
|
⟨ log(SFE) ⟩ | ||
| [M⊙] | [M⊙/L⊙] | [M⊙/kpc2] | [M⊙/Lk, ⊙ ] | [L⊙/M⊙] | [yr-1] | ||||
| median | median | median | median | median | median | median | |||
| n/nup | n/nup | n/nup | n/nup | n/nup | n/nup | n/nup | |||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | ||
|
|
|||||||||
| E-Im (T = (−5)–10) | 8.30 ± 0.08 | −1.28 ± 0.04 | 6.00 ± 0.05 | −1.87 ± 0.05 | −0.94 ± 0.05 | 0.72 ± 0.03 | −8.94 | ||
| 8.61 | −1–10 | 6.22 | −1.58 | −0.73 | 0.64 | −9.02 | |||
| 173/79 | 173/79 | 173/79 | 157/65 | 153/63 | 97/22 | 97/22 | |||
| E-Im (fap < 1.5) | 8.30 ± 0.12 | −1.29 ± 0.06 | 6.06 ± 0.07 | −1.80 ± 0.06 | −0.96 ± 0.08 | 0.80 ± 0.06 | −8.86 | ||
| 8.51 | −1.07 | 6.29 | −1.55 | −0.76 | 0.69 | −8.97 | |||
| 76/42 | 76/42 | 76/42 | 65/33 | 66/33 | 39/12 | 39/12 | |||
|
|
|||||||||
| E-S0a (T = (−5)–0) | 8.03 ± 0.12 | −1.45 ± 0.11 | 5.79 ± 0.13 | −2.32 ± 0.10 | −0.46 ± 0.21 | 0.95 ± 0.08 | −8.71 | ||
| 8.35 | −1.16 | 6.27 | −2.06 | −0.25 | 0.94 | −8.72 | |||
| 23/15 | 23/15 | 23/15 | 22/15 | 8/3 | 6/0 | 6/0 | |||
| Sa - Sab (T = 1–2) | 8.49 ± 0.18 | −1.41 ± 0.19 | 5.76 ± 0.20 | −2.27 ± 0.19 | −0.58 ± 0.21 | 0.69 ± 0.06 | −8.97 | ||
| 8.66 | −1.32 | 5.89 | −2.06 | −0.53 | 0.63 | −9.03 | |||
| 9/5 | 9/5 | 9/5 | 9/5 | 8/4 | 6/3 | 6/3 | |||
| Sb-Sc (T = 3–5) | 8.79 ± 0.06 | −1.10 ± 0.04 | 6.26 ± 0.05 | −1.66 ± 0.04 | −0.72 ± 0.06 | 0.63 ± 0.03 | −9.03 | ||
| 8.87 | −1.01 | 6.37 | −1.58 | −0.60 | 0.62 | −9.04 | |||
| 88/21 | 88/21 | 88/21 | 87/20 | 85/19 | 68/10 | 68/10 | |||
| Scd-Im (T = 6–10) | 7.78 ± 0.15 | −1.41 ± 0.05 | 5.79 ± 0.05 | −1.62 ± 0.06 | −1.38 ± 0.07 | 0.99 ± 0.09 | −8.67 | ||
| 8.26 | −1.15 | 6.01 | −1.37 | −1.07 | 0.63 | −9.03 | |||
| 53/38 | 53/38 | 53/38 | 39/25 | 52/37 | 17/9 | 17/9 | |||
Notes. Mean value and its error calculated with the program ASURV for different subsamples, and (below) median value (calculated treating the upper limits as detections). For the mean and median value of log(MH2/LFIR) and log(MH2/MHI) only galaxies with detection in LFIR or MHI, respectively, were taken into account, since ASURV cannot handle both upper and lower limits. Below: total number of galaxies and number of upper limits in MH2 taken into account for the means and median.
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