Table A.2
Main physical parameters of the LIRG and ULIRG sample derived based on the CIGALE SED-fitting code (Cols. 3–8) and CMCIRSED code (Cols. 9–12).
CIGALE | CMCIRSED | |||||||||||
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ID | z |
![]() |
log (Ldust) [L⊙] | SFR [M⊙ yr-1] | log (Mstar) [M⊙] | AGNfrac | ψ [deg] | α | χ 2 | log (Ldust) [L⊙] | T dust [K] | log (Mdust) [M⊙] |
|
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(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) | |
|
||||||||||||
2 | 0.06a | 2.85 | 11.35 ± 0.06 | 40.37 ± 5.42 | 9.90 ± 0.39 | 0.05 ± 0.00 | 26.16 | 1.57 ± 0.16 | ||||
13 | 0.20b | 4.67 | 12.02 ± 0.05 | 88.47 ± 27.79 | 11.22 ± 0.28 | 0.05 ± 0.00 | 35.96 | 1.75 ± 0.09 | 9.38 | 12.02 ± 0.00 | 25.27 ± 0.12 | 8.13 ± 0.06 |
14 | 0.22b | 1.44 | 12.04 ± 0.05 | 111.03 ± 27.73 | 10.94 ± 0.33 | 0.13 ± 0.02 | 65.57 | 1.75 ± 0.09 | 11.50 | 12.08 ± 0.01 | 29.15 ± 0.15 | 7.84 ± 0.06 |
24 | 0.16b | 4.29 | 11.56 ± 0.06 | 41.64 ± 20.00 | 10.49 ± 0.42 | 0.05 ± 0.01 | 47.01 | 1.87 ± 0.15 | 10.14 | 11.45 ± 0.05 | 33.47 ± 1.30 | 6.88 ± 0.55 |
26 | 0.38b | 0.32 | 12.31 ± 0.09 | 318.36 ± 122.24 | 11.16 ± 0.31 | 0.17 ± 0.08 | 0.92 | 1.26 ± 0.32 | ||||
46 | 0.20b | 2.29 | 11.66 ± 0.05 | 36.86 ± 8.09 | 10.80 ± 0.23 | 0.05 ± 0.00 | 73.87 | 2.06 ± 0.10 | 5.03 | 12.09 ± 0.43 | 10.08 ± 1.79 | 10.42 ± 0.09 |
47 | 0.54b | 0.63 | 12.40 ± 0.13 | 377.66 ± 148.54 | 11.18 ± 0.31 | 0.25 ± 0.08 | 0.15 | 0.96 ± 0.49 | 5.07 | 12.25 ± 0.07 | 41.74 ± 2.28 | 7.38 ± 0.08 |
59 | 0.50b | 1.54 | 12.16 ± 0.05 | 252.03 ± 56.06 | 12.26 ± 0.13 | 0.41 ± 0.03 | 0.01 | 1.76 ± 0.09 | ||||
60 | 0.14b | 1.34 | 11.11 ± 0.09 | 19.03 ± 3.66 | 10.81 ± 0.70 | 0.14 ± 0.05 | 13.32 | 1.93 ± 0.38 | ||||
61 | 0.98b | 0.81 | 12.90 ± 0.13 | 1083.40 ± 338.29 | 12.00 ± 0.30 | 0.29 ± 0.07 | 0.01 | 1.09 ± 0.43 | 6.60 | 13.07 ± 0.04 | 55.54 ± 1.68 | 7.82 ± 0.06 |
63 | 0.38b | 1.56 | 12.26 ± 0.07 | 181.03 ± 56.66 | 11.47 ± 0.25 | 0.05 ± 0.03 | 60.64 | 2.07 ± 0.10 | 12.67 | 12.78 ± 0.47 | 11.47 ± 2.34 | 10.88 ± 0.10 |
74 | 0.46b | 0.35 | 12.19 ± 0.31 | 172.68 ± 57.66 | 11.53 ± 0.44 | 0.19 ± 0.17 | 27.72 | 1.68 ± 0.28 | ||||
93 | 0.02b | 2.12 | 11.41 ± 0.05 | 32.78 ± 3.66 | 10.54 ± 0.20 | 0.13 ± 0.01 | 28.71 | 1.85 ± 0.14 | ||||
96 | 0.88b | 1.63 | 12.80 ± 0.12 | 1060.77 ± 360.17 | 11.52 ± 0.33 | 0.23 ± 0.08 | 0.03 | 0.66 ± 0.40 | 6.09 | 13.33 ± 0.14 | 14.88 ± 1.16 | 11.13 ± 0.06 |
102 | 0.52b | 1.54 | 12.30 ± 0.22 | 370.22 ± 194.25 | 10.97 ± 0.22 | 0.20 ± 0.12 | 0.18 | 0.68 ± 0.42 | 5.38 | 12.71 ± 0.16 | 17.77 ± 1.70 | 10.07 ± 0.07 |
146 | 0.10c | 1.41 | 11.18 ± 0.05 | 23.69 ± 4.82 | 11.28 ± 0.18 | 0.05 ± 0.00 | 54.05 | 2.06 ± 0.10 | 7.48 | 11.24 ± 0.09 | 34.72 ± 2.36 | 6.64 ± 0.11 |
151 | 0.54b | 1.38 | 12.17 ± 0.14 | 171.70 ± 37.43 | 11.53 ± 0.24 | 0.33 ± 0.08 | 0.01 | 2.06 ± 0.10 | 11.97 | 12.35 ± 0.02 | 38.78 ± 0.52 | 7.60 ± 0.06 |
154 | 0.24b | 1.51 | 11.40 ± 0.07 | 44.33 ± 7.73 | 11.47 ± 0.24 | 0.16 ± 0.07 | 38.45 | 2.06 ± 0.10 | 10.74 | 11.42 ± 0.02 | 34.48 ± 0.54 | 7.29 ± 0.20 |
165 | 0.36b | 3.73 | 11.85 ± 0.11 | 92.13 ± 20.98 | 11.35 ± 0.55 | 0.06 ± 0.04 | 51.86 | 2.05 ± 0.10 | ||||
175 | 0.20b | 1.47 | 11.18 ± 0.10 | 29.76 ± 7.15 | 11.35 ± 0.30 | 0.22 ± 0.10 | 40.78 | 0.82 ± 0.50 | ||||
198 | 0.60b | 0.77 | 12.36 ± 0.29 | 284.73 ± 137.47 | 11.60 ± 0.50 | 0.14 ± 0.16 | 2.84 | 1.74 ± 0.12 | 5.02 | 12.29 ± 0.10 | 44.52 ± 3.78 | 7.31 ± 0.09 |
203 | 0.13c | 1.96 | 11.64 ± 0.07 | 65.58 ± 17.02 | 10.62 ± 0.22 | 0.06 ± 0.03 | 2.82 | 1.45 ± 0.07 | 10.73 | 11.62 ± 0.04 | 34.64 ± 1.38 | 7.03 ± 0.07 |
206 | 0.92b | 1.88 | 12.68 ± 0.05 | 750.48 ± 299.76 | 11.51 ± 0.28 | 0.13 ± 0.01 | 0.07 | 1.45 ± 0.07 | 9.73 | 12.65 ± 0.02 | 36.19 ± 0.50 | 8.13 ± 0.06 |
212 | 0.74b | 0.26 | 12.70 ± 0.08 | 681.61 ± 263.71 | 11.66 ± 0.31 | 0.05 ± 0.02 | 45.80 | 2.03 ± 0.19 | ||||
215 | 0.20b | 2.33 | 11.10 ± 0.06 | 13.46 ± 3.16 | 10.39 ± 0.34 | 0.13 ± 0.01 | 61.57 | 1.87 ± 0.30 | ||||
222 | 0.62b | 3.96 | 12.02 ± 0.08 | 113.09 ± 23.50 | 11.42 ± 0.28 | 0.19 ± 0.08 | 0.02 | 1.76 ± 0.09 | ||||
234 | 0.24b | 1.80 | 11.35 ± 0.05 | 14.17 ± 2.62 | 10.63 ± 0.13 | 0.05 ± 0.01 | 82.47 | 2.06 ± 0.10 | 9.06 | 11.30 ± 0.02 | 29.28 ± 0.41 | 7.51 ± 0.08 |
251 | 0.18d | 2.78 | 11.15 ± 0.05 | 15.13 ± 4.32 | 10.33 ± 0.33 | 0.05 ± 0.01 | 62.10 | 2.06 ± 0.10 | 9.24 | 11.23 ± 0.01 | 23.42 ± 0.24 | 7.53 ± 0.06 |
252 | 0.16b | 1.03 | 11.00 ± 0.14 | 16.03 ± 4.27 | 10.96 ± 0.31 | 0.20 ± 0.08 | 87.23 | 1.76 ± 0.09 | 8.15 | 11.08 ± 0.10 | 34.40 ± 2.64 | 6.63 ± 0.22 |
260 | 0.46b | 2.36 | 11.83 ± 0.08 | 115.59 ± 13.40 | 11.65 ± 0.23 | 0.18 ± 0.07 | 4.73 | 2.08 ± 0.10 | 9.05 | 12.03 ± 0.02 | 32.55 ± 0.44 | 7.62 ± 0.06 |
265 | 0.18b | 0.73 | 11.07 ± 0.08 | 20.25 ± 5.24 | 11.22 ± 0.31 | 0.13 ± 0.03 | 86.67 | 2.21 ± 0.27 | ||||
338 | 0.24b | 4.67 | 11.05 ± 0.1 | 24.61 ± 3.85 | 10.84 ± 0.23 | 0.11 ± 0.03 | 25.28 | 2.45 ± 0.31 | 13.08 | 11.28 ± 0.02 | 26.10 ± 0.34 | 7.73 ± 0.06 |
360 | 0.26b | 2.04 | 11.18 ± 0.16 | 24.79 ± 6.15 | 11.17 ± 0.53 | 0.13 ± 0.09 | 50.71 | 1.98 ± 0.16 | 6.63 | 11.62 ± 0.37 | 16.70 ± 3.18 | 8.79 ± 0.16 |
402 | 0.64b | 3.30 | 12.30 ± 0.09 | 411.46 ± 53.08 | 12.32 ± 0.19 | 0.06 ± 0.04 | 32.24 | 2.10 ± 0.15 | ||||
443 | 0.30b | 2.58 | 11.37 ± 0.09 | 38.62 ± 5.31 | 11.20 ± 0.37 | 0.27 ± 0.06 | 10.31 | 2.09 ± 0.10 | 9.91 | 11.61 ± 0.02 | 35.53 ± 0.51 | 7.44 ± 0.58 |
466 | 0.26b | 1.52 | 11.02 ± 0.09 | 16.68 ± 2.82 | 11.60 ± 0.12 | 0.14 ± 0.05 | 73.76 | 1.89 ± 0.16 | 5.71 | 11.17 ± 0.16 | 35.86 ± 4.70 | 6.50 ± 0.11 |
610 | 0.24e | 0.29 | 11.09 ± 0.10 | 18.51 ± 2.74 | 10.89 ± 0.39 | 0.35 ± 0.04 | 0.03 | 2.11 ± 0.17 | 5.16 | 11.80 ± 0.54 | 15.94 ± 4.36 | 9.09 ± 0.18 |
618 | 0.30b | 2.93 | 11.22 ± 0.05 | 32.06 ± 2.54 | 11.38 ± 0.14 | 0.05 ± 0.00 | 42.90 | 2.21 ± 0.26 | 6.75 | 11.34 ± 0.03 | 25.33 ± 0.45 | 7.87 ± 0.07 |
837 | 1.23f | 1.03 | 13.12 ± 0.29 | 2834.36 ± 978.20 | 11.46 ± 0.69 | 0.38 ± 0.08 | 89.90 | 3.15 ± 0.47 |
Notes. Columns 2–8: CIGALE, Cols. 9–12: CMCIRSED code; (1) redshift: (2) reduced χ2; (3) dust luminosity; (4) SFR; (5) stellar mass; (6) fractional contribution of AGN MIR emission; (7) ψ – the torus angle with respect to the line of sight (Fritz et al. 2006); (8) α parameter from the Dale et al. (2014) model; (9) reduced χ2; (10) dust luminosity; (11) dust temperature; (12) dust mass.
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