Table 2.
Comparison of the main properties of the [Ne V] sample and of the control sample.
[Ne V] | Control | |
---|---|---|
z | ![]() |
0.85 ± 0.11 |
log(M*/M⊙) | ![]() |
![]() |
SFRsed (M⊙ yr−1) | ![]() |
![]() |
log(sSFR/yr−1) | ![]() |
![]() |
SFRnorm | ![]() |
![]() |
fMS | ![]() |
0.30 ± 0.01 |
log(Mmolgas/M⊙) | ![]() |
![]() |
fmol | ![]() |
![]() |
log(tage/yr−1) | ![]() |
![]() |
log(MBH/M⊙) | ![]() |
|
λEdd | ![]() |
Notes. We report the median values (with the 16th and 84th percentiles) for the redshift z, stellar mass, SFR, specific SFR (sSFR = SFR/M*), SFRnorm = SFR/SFRMS, fraction of sources within the Schreiber et al. (2015) MS (fMS), molecular gas mass (Mmolgas), the molecular gas fraction (fmol = Mmolgas/(Mmolgas + M*)), age of the galaxy (tage, from the SED-fitting), BH mass (MBH), and Eddington ratio (λEdd).
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