Table 3.
Ratio (without unit) between the monochromatic continuum luminosity νLν and the total infrared luminosity LIR at different rest-frame wavelengths associated with important far-IR lines.
[OI]63 | [OIII] | [NII]122 | [OI]145 | [CII] | [NII]205 | |
---|---|---|---|---|---|---|
Rest-frame wavelength (μm) | 63 | 88 | 122 | 145 | 158 | 205 |
νLν/LIR from B17 | 0.69 | 0.50 | 0.27 | 0.18 | 0.133 | 0.054 |
νLν/LIR from S18 | 0.64 | 0.43 | 0.20 | 0.12 | 0.093 | 0.038 |
νLν/LIR for 40 K MBB | 0.93 | 0.69 | 0.34 | 0.20 | 0.155 | 0.062 |
νLν/LIR for 45 K MBB | 0.89 | 0.55 | 0.24 | 0.14 | 0.104 | 0.040 |
νLν/LIR for 50 K MBB | 0.81 | 0.44 | 0.17 | 0.10 | 0.071 | 0.026 |
νLν/LIR for 55 K MBB | 0.71 | 0.34 | 0.13 | 0.07 | 0.050 | 0.018 |
νLν/LIR for 60 K MBB | 0.60 | 0.27 | 0.09 | 0.05 | 0.036 | 0.013 |
Notes. These ratios were computed using the Bethermin et al. (2017, B17) z > 4 and Schreiber et al. (2018, S18) main-sequence SED templates and modified blackbodies (MBBs) at various rest-frame temperatures (β fixed to 1.8) for comparison.
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