Table 2.
Comparison of kIR values obtained for the Auriga-D sample and the observational sample considered in this work.
| Band | ⟨kIR⟩fR, opt = 1 | ⟨kIR⟩LIRfR, opt = 1 | ⟨kIR⟩f R, opt = 0.33 | ⟨kIR⟩LIRf R, opt = 0.33 | ⟨kIR⟩, B16 | ⟨kIR⟩LIR, B16 | kIR, H11 | kIR, L11 |
|---|---|---|---|---|---|---|---|---|
| 24 | 7.95 ± 4.25 | 7.43 ± 2.83 | 6.12 ± 2.72 | 6.25 ± 1.91 | 8.11 ± 2.10 | 6.17 ± 2.17 | 3.89 ± 0.15 | 6.0 |
| 70 | 1.03 ± 0.30 | 0.83 ± 0.30 | 0.81 ± 0.28 | 0.65 ± 0.25 | 1.57 ± 0.39 | 1.12 ± 0.50 | – | – |
| TIR | 0.50 ± 0.15 | 0.43 ± 0.15 | 0.36 ± 0.14 | 0.33 ± 0.11 | 0.63 ± 0.12 | 0.58 ± 0.12 | 0.46 ± 0.12 | – |
Notes. The first four columns show the mean kIR values for the Auriga-D sample, obtained across three bands and using three different face-on galaxy inclinations. The superscripts in these columns represent the aperture, while the subscripts, when present, indicate the luminosity weighting in the average. Cols. 5 and 6 display corresponding results for the B16 dataset, while the final two columns report values from H11 and L11 studies.
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