Table 3.
GS-14 properties from photometric and spectral analyses.
Photometric | Spectral | |
---|---|---|
![]() |
![]() |
|
![]() |
![]() |
|
![]() |
8.7 ± 0.1 |
![]() |
age![]() |
680 ± 170 | |
age![]() |
8 ± 6 | 2.7 ± 0.1 |
SFR (M⊙/yr) | 90 ± 30 | |
SFRMS (M⊙/yr) | ∼200 | |
SFR[C II] (M⊙/yr) |
![]() |
|
SFRUV (M⊙/yr) | 26 ± 5 | |
Z/Z⊙ | < 0.2 | 0.5 |
fmol |
![]() |
|
E(B − V) | 0.05 | 0.05 |
![]() |
< 44.5 | |
![]() |
< 43.5 |
Notes. ,
, and
refer to the total, old, and young population, respectively. age
and age
refer to the age of the old and young stellar population. SFR refers to the instantaneous SFR from the SED fitting, SFRMS to the expected SFR for an MS galaxy of similar mass and redshift, obtained using the Speagle et al. (2014) MS, SFR[C II] refers to the SFR estimated from the [C II] luminosity and using the Schaerer et al. (2020) relations of Fig. 3, and SFRUV to the SFR obtained from the UV luminosity. Z refers to the metallicity. The molecular gas fraction fmol was computed with the Mmolgas of Dessauges-Zavadsky et al. (2020). The E(B − V) in the Photometric column was derived from the SED fitting by Faisst et al. (2020), while the one in the Spectral column from the VIMOS spectrum as described in Sect. 2.2.
and
are the AGN bolometric luminosity derived from the SED fitting and from the Chandra X-ray flux upper limit, assuming the bolometric correction from Lusso et al. (2012), respectively.
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.