Free Access

Table 3.

Main physical properties of the sample of 42 453 galaxies presented in total IR luminosity bins.

Ngal NAGN Redshift log(Mstar) log(SFR) log(sSFR)
(%) (%) (M (M yr−1) (yr−1)
(1) (2) (3) (4) (5) (6) (7)
log(Ldust) < 11 6974 268 0.42 ± 0.15 10.12 ± 0.34 0.64 ± 0.27 −9.70 ± 0.16
16.43% 3.86%
LIRGs 11 ≤ log(Ldust) < 12 23 214 724 0.96 ± 0.27 10.73 ± 0.24 1.59 ± 0.23 −9.22 ± 0.31
54.68% 3.11%
ULIRGs 12 ≤ log(Ldust) < 13 11 947 705 1.89 ± 0.32 11.10 ± 0.22 2.30 ± 0.17 −8.85 ± 0.21
28.14% 5.90%
HLIRGs log(Ldust) ≽ 13 318 65 4.92 ± 0.34 11.49 ± 0.34 3.52 ± 0.17 −8.01 ± 0.53
0.75% 20.44%

Notes. The first column corresponds to the galaxy type according to their total log(Ldust) value, the second shows the number of galaxies (first row), and the total percentage of the sample (second row), Col. (3) presents the number of galaxies with an AGN contribution higher than 20% (first row – total number, second row – percentage value of galaxiwhiches with AGN contribution within the given IR luminosity bin). Median values for redshift, stellar mass, SFR and specific SFR are given in Cols. (4)–(7). The errors are calculated as median absolute deviation.

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.