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Table 1:

Mean values for SMGs in redshift bins.
  Volume $\log\rho_{\rm IR}$ $\rho_{\rm SFR}$   $\log\rho_{*}$     $\log\rho_{\rm dust}$
z (106 Mpc3) $(L_\odot~\mbox{Mpc}^{-3})$ $(M_\odot~\mbox{yr}^{-1}~\mbox{Mpc}^{-3})$ % $(M_\odot~\mbox{Mpc}^{-3})$ % q $(M_\odot~\mbox{Mpc}^{-3})$
(1) (2) (3) (4) (5) (6) (7) (8) (9)
0.080-0.500 0.12 $7.03_{\rm -0.14}^{+0.11}$ $0.0018\pm0.0005$ $ 5_{\rm - 2}^{+ 3}$ $6.35_{\rm -0.16}^{+0.21}$ $ 1_{\rm - 0.2}^{+ 0.4}$ $2.54\pm 0.12$ $ 4.06_{\rm -0.06}^{+0.05}$
0.510-1.316 1.03 $7.81_{\rm -0.07}^{+0.06}$ $0.0111\pm0.0016$ $ 9_{\rm - 2}^{+ 2}$ $7.16_{\rm -0.08}^{+0.13}$ $ 5_{\rm - 1}^{+ 2}$ $2.52\pm 0.06$ $ 4.32_{\rm -0.05}^{+0.04}$
1.408-2.142 1.63 $8.12_{\rm -0.05}^{+0.05}$ $0.0228\pm0.0027$ $ 11_{\rm - 3}^{+ 3}$ $7.18_{\rm -0.11}^{+0.16}$ $ 11_{\rm - 3}^{+ 6}$ $2.29\pm 0.08$ $3.84_{\rm -0.04}^{+0.04}$
2.148-2.565 0.89 $8.45_{\rm -0.05}^{+0.05}$ $0.0486\pm0.0054$ $ 18_{\rm - 5}^{+ 7}$ $7.61_{\rm -0.08}^{+0.12}$ $ 51_{\rm - 11}^{+ 20}$ $2.27\pm 0.09$ $4.35_{\rm -0.04}^{+0.04}$
2.578-3.623 2.17 $8.30_{\rm -0.05}^{+0.05}$ $0.0341\pm0.0040$ $ 20_{\rm - 4}^{+ 5}$ $7.28_{\rm -0.07}^{+0.12}$ $ 31_{\rm - 7}^{+14}$ $2.25\pm 0.08$ $3.86_{\rm -0.03}^{+0.03}$

Notes. Column (1): redshift range of the bins. Column (2): comoving volume of these bins (calculated in Sect. 3.2). Column (3): IR luminosty density of SMGs. Column (4): Resulting IR SFR density of SMGs (Sect. 5.3.1). Column (5): contribution of SMGs to the cosmic SFR density (calculated in Sect. 3.2). Column (6): stellar mass density of SMGs (Sect. 5.3.2). Column (7): contribution of SMGs to the cosmic M* density (calculated in Sect. 3.2). Column (8): mean (and error of the mean) IR-radio correlation parameter for SMGs (Sect. 5.4.1). Column (9): dust mass density of SMGs (Sect. 5.2.3). Columns (3-7) and (9) have been corrected for incompleteness by a factor of 3.5 (Sect. 3.2).


Source LaTeX | All tables | In the text

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