Table 3
Reconstructed emissivity as a function of redshift and associated star formation rate.
| 1 <z ≤ 1.5 | 1.5 <z ≤ 3 | 3 <z ≤ 7 | |||||||||
|
ρ SFR |
|
ρ SFR |
|
ρ SFR | ||||||
|
|
|||||||||||
| 100 GHz ..... | 7.2 ± 5.8 | 1.96 ± 1.58 | 3.5 ± 3.0 | 0.66 ± 0.56 | 5.5 ± 4.8 | 0.27 ± 0.24 | |||||
| 143 GHz ..... | 12.7 ± 9.6 | 1.37 ± 0.96 | 6.8 ± 5.5 | 0.44 ± 0.35 | 10.5 ± 9.0 | 0.18 ± 0.15 | |||||
| 217 GHz ..... | 11.9 ± 6.3 | 0.31 ± 0.16 | 17.3 ± 7.2 | 0.28 ± 0.12 | 36.6 ± 13.8 | 0.18 ± 0.07 | |||||
| 353 GHz ..... | 116? ± 17? | 0.67 ± 0.10 | 75.5 ± 27.5 | 0.29 ± 0.10 | 164? ± 47? | 0.32 ± 0.09 | |||||
| 545 GHz ..... | 185? ± 106? | 0.32 ± 0.18 | 224? ± 148? | 0.32 ± 0.21 | 417? ± 251? | 0.66 ± 0.40 | |||||
| 857 GHz ..... | 193? ± 139? | 0.14 ± 0.10 | 354? ± 212? | 0.32 ± 0.19 | 609? ± 359? | 1.37 ± 0.81 | |||||
Notes. At each frequency and for each of the three redshift bins the
first quantity corresponds to the mean emissivity in the corresponding redshift bin,
,
in Jy Mpc-1
sr-1, while the second corresponds to the SFR density,
ρSFR, in M⊙ Mpc-3
yr-1.
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