Open Access

Table 1.

Measurements and physical properties.

Property NS_274 RUBIES-UDS-QG-z7
RA [deg] 171.8236199 34.4296173
Dec [deg] 42.4696455 –5.1122962
zspec 4.1061±0.0003 7.2758±0.0011
μ 2.0±0.2 1
μ [Ne III]λ3870 [10−19 cgs] 2 . 4 2.4 + 2.8 $ 2.4^{+2.8}_{-2.4} $
μ [O II]λ3729 [10−19 cgs] <6.6
μ Hβ λ4863 [10−19 cgs] 8 . 0 3.8 + 3.7 $ 8.0^{+3.7}_{-3.8} $
μ [O III]λ5008 [10−19 cgs] 8 . 9 4.2 + 3.9 $ 8.9^{+3.9}_{-4.2} $
μ mF200W,AB [mag] 23.34±0.05 26.31±0.06
log(M/M) 10 . 57 0.02 + 0.02 $ 10.57^{+0.02}_{-0.02} $ 10 . 13 0.02 + 0.07 $ 10.13^{+0.07}_{-0.02} $
AV [mag] 0 . 40 0.04 + 0.04 $ 0.40^{+0.04}_{-0.04} $ 0 . 50 0.10 + 0.06 $ 0.50^{+0.06}_{-0.10} $
SFR100 Myr [M yr−1] 10 . 7 0.1 + 0.1 $ 10.7^{+0.1}_{-0.1} $ 33 32 + 93 $ 33^{+93}_{-32} $
SFR10 Myr [M yr−1] 9 . 0 0.1 + 0.1 $ 9.0^{+0.1}_{-0.1} $ <2
SFRIR, 8−1000 μm [M yr−1] <12
SFR[OII] [M yr−1] <0.4
SFRHβ [M yr−1] 1 . 5 0.7 + 0.7 $ 1.5^{+0.7}_{-0.7} $
log(sSFR100 Myr/yr−1) 9 . 54 0.05 + 0.05 $ -9.54^{+0.05}_{-0.05} $ 8 . 7 1.9 + 0.6 $ -8.7^{+0.6}_{-1.9} $
σ [km s−1] 255 42 + 39 $ 255^{+39}_{-42} $
Δvoff [km s−1] −182±50 −169±46
Rmaj [pc] 262 15 + 17 $ 262^{+17}_{-15} $ 209 24 + 33 $ 209^{+33}_{-24} $
nSersic 6 . 5 0.5 + 0.6 $ 6.5^{+0.6}_{-0.5} $ 2 . 4 0.9 + 1.5 $ 2.4^{+1.5}_{-0.9} $
log(Mdyn/M) 10 . 18 0.16 + 0.13 $ 10.18^{+0.13}_{-0.16} $

log(N(FeII)/cm−2) 15.00±0.19
log(N(MgII)/cm−2) 15.35±0.74 ∼17.9
log(N(NaI)/cm−2) 12.15±0.59
log(N(HFe)/cm−2) 21.19±0.19
log(N(HMg)/cm−2) 20.57±0.74 ∼23.1
log(N(HNa)/cm−2) 19.79±0.59
out [M yr−1] (Fe, Mg, Na) ( 5 3 + 5 , 1 1 + 7 , 0 . 2 0.2 + 0.8 ) $ (5^{+5}_{-3},\,1^{+7}_{-1},\,0.2^{+0.8}_{-0.2}) $ (−,∼269,−)
η (Fe, Mg, Na) ( 0 . 2 0.1 + 0.3 , 0 . 1 0.1 + 0.4 , 0 . 01 0.01 + 0.04 ) $ (0.2^{+0.3}_{-0.1},\,0.1^{+0.4}_{-0.1},\,0.01^{+0.04}_{-0.01}) $ (−,∼12,−)

Notes. Upper limits at 3σ. The [Ne III], [O II], Hβ, and [O III] fluxes refer to emission lines obtained after subtracting the underlying stellar continuum. out and η are computed assuming voutvoff and SFR100 Myr (Sect. 4 for a discussion of alternative options).

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