Table A.5
Evolution of the comoving IR energy density and the relative contribution of “faint” galaxies (107 L⊙ < LIR < 1011 L⊙), LIRGs (1011 L⊙ < LIR < 1012 L⊙) and ULIRGs (LIR > 1012 L⊙).
| Redshift | Total IR LD | “faint” galaxies | LIRGs | ULIRGs |
| [106 × L⊙ Mpc-3] | [106 × L⊙ Mpc-3] | [106 × L⊙ Mpc-3] | [106 × L⊙ Mpc-3] | |
|
|
||||
| 0.00a |
|
|
|
|
| 0.25 |
|
|
|
|
| 0.55 |
|
|
|
|
| 0.85 |
|
|
|
|
| 1.15 |
|
|
|
|
| 1.55 |
|
|
|
|
| 2.05 |
|
|
|
|
Notes.The local reference is taken from Sanders et al. (2003). Comoving infrared energy densities constrained using our PACS observations are highlighted in bold. Others values rely upon extrapolations based on φknee and Lknee and a faint-end slope of the IR LF fixed at its z ~ 0 value.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.