Table 2.
Cosmic dust mass density derived from the ALPINE survey at z ∼ 5.
| log(ρdust) z ∼ 5 | |
|---|---|
| log(ρdust, UV) | log(ρdust, IR) |
| [M⊙ Mpc−3] | [M⊙ Mpc−3] |
4.8 |
5.3 |
| > 4.3 | > 4.8 |
Notes. The left column lists the measurement derived from the ALPINE UV-selected galaxies using LUV as proxy for Mdust and integrating the UVLF in the typical 0.03L⋆ − 100L⋆ range. The right column lists the measurement derived from the serendipitous IR-detected sources using LIR as proxy for Mdust and integrating the IRLF in the typical 9 < log(LIR) < 14 range. We also report in the second row the lower limits obtained by integrating the UVLF and IRLF only in the range sampled by the detected sources (10.4 < log(LUV) < 11.5 and 11.2 < log(LIR) < 13, respectively).
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