Table 5
Values of the aIR coefficients for the calibration of hybrid tracers: by stellar mass (see Sects. 4.5.2 and 4.5.4 for a detailed explanation).
| Without type-2 AGN | With type-2 AGN | |||||||
| Hybrid tracers |
|
|||||||
| log[M⋆] > 10.5 | 10.0 < log[M⋆] < 10.5 | log[M⋆] < 10.0 | log[M⋆] > 10.5 | 10.0 < log[M⋆] < 10.5 | log[M⋆] < 10.0 | |||
|
|
||||||||
| L(Hα)obs + aIR×L(22 μm) | 0.014 [44] |
0.021 [60] |
0.021 [60] |
0.009 [108] |
0.017 [88] |
0.019 [66] |
||
| L(Hα)obs + aIR×L(TIR) | 0.0018 [37] |
0.0020 [54] |
0.0021 [44] |
0.0010 [92] |
0.0018 [77] |
0.0019 [48] |
||
| L(FUV)obs + aIR×L(22 μm) | 4.06 [30] |
4.75 [39] |
4.77 [44] |
2.93 [81] |
4.25 [57] |
4.55 [48] |
||
| L(FUV)obs + aIR×L(TIR) | 0.36 [26] |
0.44 [36] |
0.41 [32] |
0.25 [70] |
0.41 [50] |
0.40 [35] |
||
Notes. The stellar masses are in units of M⋆/M⊙. Expressions to compute the SFR (M⊙ yr-1) appeared in the left column. These recipes are the same as those in Table 3. The luminosities are in units of erg s-1.
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