Table 1.
Infrared luminosity function as inferred using the A3COSMOS database.
| log(LIR/L⊙) | log(Φ/Mpc−3 dex−1) |
|||
|---|---|---|---|---|
| 0.5 < z ≤ 1.0 | 1.0 < z ≤ 1.5 | 1.5 < z ≤ 2.0 | 2.0 < z ≤ 2.5 | |
| 11.25-11.75 | (−4.54 ± 0.71 [3]) | (−4.61 ± 0.41 [8]) | ||
| 11.50–12.00 | (−4.54 ± 0.71 [2]) | (−4.12 ± 0.41 [9]) | (−4.03 ± 0.35 [9]) | (−4.46 ± 0.38 [7]) |
| 11.75–12.25 | −4.44 ± 1.00 [1] | (−3.95 ± 0.41 [9]) | (−3.43 ± 0.32 [12]) | (−4.08 ± 0.38 [7]) |
| 12.00–12.50 | −4.17 ± 0.71 [2] | −3.97 ± 0.41 [8] | −3.31 ± 0.22 [21] | −3.79 ± 0.27 [14] |
| 12.25–12.75 | −4.50 ± 1.00 [1] | −4.32 ± 0.50 [5] | −3.62 ± 0.22 [20] | −3.68 ± 0.24 [17] |
| 12.50–13.00 | −4.99 ± 0.71 [2] | −4.38 ± 0.5 [4] | −3.90 ± 0.29 [12] | |
| 12.75–13.25 | −4.99 ± 1.00 [1] | −5.14 ± 1.00 [1] | −4.48 ± 0.50 [4] | |
| 2.5 < z ≤ 3.0 | 3.0 < z ≤ 3.5 | 3.5 < z ≤ 4.5 | 4.5 < z ≤ 6.0 | |
| 11.25–11.75 | (−4.67 ± 0.71 [2]) | |||
| 11.50–12.00 | (−4.93 ± 0.58 [3]) | (−4.76 ± 1.00 [1]) | (−4.53 ± 0.50 [3]) | (−5.21 ± 0.58 [2]) |
| 11.75–12.25 | (−4.04 ± 0.30 [11]) | (−4.27 ± 0.45 [3]) | (−4.85 ± 0.58 [2]) | (−4.81 ± 0.58 [3]) |
| 12.00–12.50 | −3.76 ± 0.25 [16] | −3.91 ± 0.30 [9] | −4.42 ± 0.41 [6] | −4.60 ± 0.45 [5] |
| 12.25–12.75 | −3.87 ± 0.28 [13] | −3.83 ± 0.29 [13] | −4.29 ± 0.35 [8] | −4.64 ± 0.41 [6] |
| 12.50–13.00 | −4.07 ± 0.29 [12] | −4.03 ± 0.32 [11] | −4.48 ± 0.41 [6] | −5.01 ± 0.58 [3] |
| 12.75–13.25 | −4.28 ± 0.35 [8] | −4.47 ± 0.45 [5] | −4.59 ± 0.41 [7] | −5.25 ± 0.71 [2] |
| 13.00–13.50 | −5.19 ± 1.00 [1] | −4.93 ± 0.58 [4] | −5.58 ± 1.00 [1] | |
Notes. In the first column, the luminosity bins are reported, while Cols. 2–8 report the Φ values in each luminosity and redshift bins. Bold (or italic) values represent independent luminosity bins. Values in round brackets indicate luminosity bins that are below the completeness limit, and numbers in square brackets are the number of sources in each L-z bin.
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