Table 2.
Modes and 68% percentiles for the logarithm of the ratio between the estimated SFR for the model SEDs using Eq. (4), based on WISE band-1 and band-3 or NIR-F200W and MIRI-F2100W, over the true SFR as given by the SFHs of the SED modeling.
 |
||||
|---|---|---|---|---|
| SFR range |
 |
 |
||
| E(B − V) distribution | Uniform | SDSS | Uniform | SDSS |
| [W1, W3] |
 |
 |
 |
 |
| [W1, W3, E(B − V)] |
 |
 |
 |
 |
| [W1, W3, IRXu] |
 |
 |
 |
 |
| [W1, W3, IRXg] |
 |
 |
 |
 |
| [F200W, F2100W] |
 |
 |
 |
 |
| [F200W, F2100W, E(B − V)] |
 |
 |
 |
 |
| Jarrett et al. (2013) [W3] |
 |
 |
 |
 |
| Chang et al. (2015) [W3] |
 |
 |
 |
 |
| Cluver et al. (2017) [W3] |
 |
 |
 |
 |
Notes. Similarly, estimations based on WISE band-3 for the relations of Jarrett et al. (2013), Chang et al. (2015), and Cluver et al. (2017) are given. The two columns are for comparisons using the uniform-E(B − V) samples, and the SDSS-matched E(B − V) samples in the SFR range −4 < logSFR/M⊙ yr−1) < − 1 (left), and −1 < log(SFR/M⊙ yr−1) (right).
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