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Table 4.
Star formation rate density obtained by integrating the LF best-fit in our eight redshift bins.
| z | log ρSFR | log ρSFR | log ρSFR |
|---|---|---|---|
| [M⊙ yr−1 Mpc−3] | |||
| 50th | 16th | 84th | |
| 0.5 − 1.0 | −1.25 | −1.27 | −1.23 |
| 1.0 − 1.5 | −1.17 | −1.20 | −1.15 |
| 1.5 − 2.0 | −1.16 | −1.19 | −1.14 |
| 2.0 − 2.5 | −1.16 | −1.20 | −1.13 |
| 2.5 − 3.0 | −1.17 | −1.23 | −1.12 |
| 3.0 − 3.5 | −1.19 | −1.29 | −1.12 |
| 3.−4.5 | −1.40 | −1.53 | −1.24 |
| 4.5 − 6.0 | −1.67 | −1.92 | −1.32 |
Notes. The second column is the median value, while third and fourth columns show the lower and upper 16th boundaries.
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