Table 4.
Average emission line luminosities for galaxies at z ∼ 1.25.
| Main sequence | |||
|---|---|---|---|
| Transition | Ndet, Nup | Mean | Median (a) |
 |
18, 4 | 1.83 ± 0.23 ( † ) |
 |
 |
4, 0 | 0.66 ± 0.08 |
 |
 |
20, 2 | 0.52 ± 0.06 ( † ) |
 |
 |
6, 0 | 0.17 ± 0.04 |
 |
 |
7, 1 | 0.37 ± 0.05 ( † ) |
 |
 |
6, 0 | 0.17 ± 0.03 |
 |
| Starbursts | |||
| Transition | Ndet, Nup | Mean | Median (a) |
 |
11, 1 | 1.91 ± 0.24 ( † ) |
 |
 |
− | − | − |
 |
15, 0 | 0.62 ± 0.08 |
 |
 |
6, 0 | 0.22 ± 0.05 |
 |
 |
− | − | − |
 |
6, 0 | 0.20 ± 0.04 |
 |
| Extreme starbursts | |||
| Transition | Ndet, Nup | Mean | Median (a) |
 |
6, 1 | 1.80 ± 0.27 ( † ) |
 |
 |
− | − | − |
 |
6, 0 | 0.72 ± 0.12 |
 |
 |
3, 0 | 0.31 ± 0.06 | − |
 |
− | − | − |
 |
3, 0 | 0.27 ± 0.06 | − |
Notes. The L′ luminosities are expressed in 1010 K km s−1 pc2. The average I fluxes in Jy km s−1 shown in Figs. 8 and 9 are computed adopting z = 1.25. The main sequence is parameterized as in Sargent et al. (2014). Galaxies are defined as starbursts if ΔMS ≥ 3.5 and extreme starbursts if ΔMS ≥ 7. ( † )Formally biased mean value, as the first upper limit was turned into a detection for the calculation of the KM estimator (Kaplan & Meier 1958).
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