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Home All issues Volume 618 (October 2018) A&A, 618 (2018) A85 Full HTML
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Table A6.

Summary of SFR estimates from SED modeling or emission lines.

ID SFR10a Line b c
M⊙ yr−1 M⊙ yr−1 M⊙ yr−1
Confirmed z > 3 galaxies
ZF-COS-17779 Hβ 3.4 ± 0.8
... ... [O II] 1.1 ± 0.6
ZF-COS-18842 Hβ 3.6 ± 8.9
... ... [O II] 0.0 ± 1.9
ZF-COS-19589 Hβ 3.8 ± 5.6
ZF-COS-20115 Hβ 0.0 ± 1.8
... ... [O II] 0.0 ± 1.6
ZF-COS-20133 Hβ 11.2 ± 1.1
... ... [O II] 0.0 ± 0.8
3D-EGS-18996 Hβ 0.0 ± 1.9
... ... [O II] 3.6 ± 2.0
3D-EGS-26047 Hβ 36.0 ± 17.0
... ... [O II] 6.8 ± 2.6
3D-EGS-31322 Hβ 11.9 ± 8.8
... ... [O II] 3.6 ± 2.3
3D-EGS-40032 Hβ 5.6 ± 5.4
... ... [O II] 10.3 ± 2.3
ZF-UDS-8197 Hβ 4.0 ± 4.1
... ... [O II] 0.0 ± 0.2
Interlopers at z < 3
ZF-COS-20032 Hα 3.9 ± 1.5
... ... Hβ 1.0 ± 2.7
3D-UDS-27939 Hα 12.8 ± 0.9
(a)

Notes. SFR estimated from the SED modeling, averaged over the last 10 Myr preceeding observation.

(b)

SFR estimated from the observed emission line luminosity, without correcting for dust attenuation.

(c)

Same, but corrected for dust attenuation using the best-fit AV from the SED modeling.

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