Fig. 13

Left: relation between the
L[C II ] ∕LFIR
ratio and LFIR.
The values observed for Hyde are shown with
a green square. The range of values found in
z = 0
luminous infrared galaxies are indicated with
the hashed region (Díaz-Santos et al. 2013).
High-redshift galaxies from the literature are
shown with colored circles: light blue for the
z = 2
galaxies of Brisbin et al. (2015), dark blue for the lensed
z = 2
galaxy studied in Schaerer et al. (2015), red for the
z = 4.5
SMGs found near quasars in
Trakhtenbrot et al. (2017), purple for the
z = 5
LBGs of Capak et al. (2015), and
finally orange a collection of galaxies at
z = 3–5
(Cox et al. 2011; De Breuck et al. 2011; Valtchanov et al. 2011; Swinbank et al. 2012; Walter et al. 2012; Wagg et al. 2012; Riechers et al. 2013, 2014; Gullberg et al. 2015; Oteo et al. 2016). Galaxies from Brisbin et al.(2015)
and Gullberg et al.(2015) with unknown
magnification factors were assumed to have
μ = 10
(the average of the published magnifications
from both samples). When needed, we assumed
LFIR = LIR∕1.5.
Right: relation between the offset from the main sequence
(SFR ∕SFRMS)
and the stellar mass for the galaxies on the
left with measured masses. If no stellar mass
estimate was available, we inferred it from the
dynamical mass assuming a gas fraction of
50%.
The value of SFRMS
was taken from Schreiber et al. (2015) at
z < 3.5
and Schreiber et al. (2017) at
3.5 ≤ z ≤ 4.5;
values at higher redshifts were estimated
assuming a redshift dependence of
.
On this plot, we also show with purple circles the two
z = 6.6
LBGs of Smit et al. (2018), which are detected in [C II]
but not in the FIR continuum, and thus for which the
SFR
is based only on the UV luminosity.
We also show the position of
z = 4
main sequence galaxies from Schreiber et al. (2017)
as small green squares; these galaxies have
no [C II] measurement. The 90% confidence
region for Hyde is shown in light green, and
the most conservative upper limit of Jekyll
(SFR < 13 M⊙
yr−1
at 3σ,
as obtained from SFRIR)
is shown with a blue arrow for reference.
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