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Table 2.

Physical properties of our sample of galaxies.

Source z[CII] log(M*) log(SFR[CII]) log(MH2, TOT) 12 + log(O/H)
[M] [M yr−1] [M]
(1) (2) (3) (4) (5) (6)
Haro2 0.0049 8.23 ± 0.03
Haro3 0.0032 8.28 ± 0.01
Haro11 0.0207 8.36 ± 0.01
He2-10 0.0029 8.43 ± 0.01
HS0052+2536 0.0462 8.07 ± 0.20
HS1222+3741 0.0405 7.79 ± 0.01
HS1304+3529 0.0162 7.93 ± 0.10
HS1330+3651 0.0165 7.98 ± 0.10
HS1442+4250 0.0022 7.60 ± 0.01
HS2352+2733 0.0273 8.40 ± 0.20
IZw18 0.0025 7.14 ± 0.01
IIZw40 0.0026 8.23 ± 0.01
Mrk153 0.0080 7.86 ± 0.04
Mrk209 0.0010 7.74 ± 0.01
Mrk930 0.0183 8.03 ± 0.01
Mrk1089 0.0134 8.10 ± 0.08
Mrk1450 0.0032 7.84 ± 0.01
SBS0335–052 0.0136 7.25 ± 0.01
SBS1159+545 0.0121 7.44 ± 0.01
SBS1211+540 0.0030 7.58 ± 0.01
SBS1249+493 0.0248 7.68 ± 0.02
SBS1415+437 0.0021 7.55 ± 0.01
SBS1533+574 0.0114 8.05 ± 0.01
UGC4483 0.0006 7.46 ± 0.02
UM133 0.0053 7.82 ± 0.01
UM311 0.0057 8.36 ± 0.01
UM448 0.0184 8.32 ± 0.01
UM461 0.0034 7.73 ± 0.01
VIIZw403 −0.0002 7.66 ± 0.01

Notes. Column key: (1) source name; (2) redshift based on [CII] emission line; (3) stellar mass from CIGALE; (4) SFR from [CII] emission; (5) mass of total molecular gas estimated from [CII] luminosity; (6) metallicity values in 12 + log(O/H) from Madden et al. (2013). SFRs and MH2, TOT were obtained from the [CII] luminosity of the narrow components following the relations found by De Looze et al. (2014) and Madden et al. (2020) for the DGS galaxies, respectively. The typical z[CII] uncertainties based on the spectral resolution are 0.0001.

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