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Table 6.

Physical properties for our sources derived through SED fitting.

ID log(M) log(SFR) log(LIR) AV log( M H 2 CO $ M^{\mathrm{CO}}_{\mathrm{H}_2} $) log( M H 2 [ CI ] $ M^{[\mathrm{CI}]}_{\mathrm{H}_2} $) τD(a)
[M] [M yr−1] [L] [mag] [M] [M] [Myr]
RSN-41 11.0 ± 0.1 2.72 ± 0.06 12.56 ± 0.06 4.9 ± 0.2 11.10 ± 0.06 242 ± 50
RSN-84 11.0 ± 0.1 2.76 ± 0.03 12.57 ± 0.03 4.8 ± 0.2 10.86 ± 0.08 11.17 ± 0.06 258 ± 53
RSN-121 11.0 ± 0.1 2.65 ± 0.06 12.47 ± 0.06 4.2 ± 0.2 11.11 ± 0.07 11.01 ± 0.07 229 ± 60
RSN-182 11.1 ± 0.1 2.92 ± 0.03 12.72 ± 0.03 3.8 ± 0.2 11.02 ± 0.08 126 ± 27
RSN-235 11.3 ± 0.1 3.04 ± 0.03 12.83 ± 0.04 4.5 ± 0.2 11.07 ± 0.08 10.96 ± 0.08 83 ± 18
RSN-247 10.7 ± 0.2 2.57 ± 0.04 12.46 ± 0.04 4.6 ± 0.4 10.71 ± 0.09 140 ± 31
RSN-298 11.0 ± 0.1 2.69 ± 0.06 12.58 ± 0.06 4.2 ± 0.3 10.81 ± 0.08 132 ± 30
RSN-361 10.8 ± 0.3 2.79 ± 0.03 12.61 ± 0.03 3.9 ± 0.6 10.7 ± 0.1 11.06 ± 0.06 186 ± 34
RSN-456 10.8 ± 0.2 2.41 ± 0.07 12.37 ± 0.07 4.6 ± 0.3 10.93 ± 0.06 288 ± 63

Median (b) 11.0 ± 0.1 2.6 ± 0.1 12.6 ± 0.1 4.5 ± 0.4 10.9 ± 0.2 11.03 ± 0.07 263 ± 86

G24 (b) 11.0 ± 0.4 2.8 ± 0.4 12.6 ± 0.4 3.9 ± 0.3

Notes. The SED fitting is performed with the code CIGALE (Boquien et al. 2019) after the assumed spectroscopic redshifts were retrieved in Sect. 3.3. The last two columns report the molecular gas mass and the depletion time as estimated in Sect. 4.3. The last two rows report the median value computed for the galaxies here and for the whole sample analyzed in Gentile et al. (2024) with CIGALE.

(a)

Estimated from the M H 2 [ CI ] $ M^{[\mathrm{CI}]}_{\mathrm{H}_2} $ when available.

(b)

The uncertainties on the median quantities are reported as half the interval between the 84th and the 16th percentile.

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