Table 2.
Targets with the best attenuation laws used to fit the full SED.
| ID | CLS ID | Redshift | Best law |  |
Other laws |
|---|---|---|---|---|---|
| GS01* | 3280 | 2.191 | C00 | 21.0 | LF17 |
| GS02 | 5339 | 2.326 | CF00 | 49.0 | LF17 |
| GS03* | 2619 | 2.241 | LF17 | 15.7 | CF00 |
| GS04 | 7184 | 1.956 | CF00 | 37.2 | LF17 |
| GS05* | 9834 | 2.576 | LF17 | 43.3 | |
| GS06* | 14876 | 2.309 | LF17 | 54.1 | |
| GS07* | 8409 | 1.619 | CF00 | 52.9 | |
| UDF1* | 15669 | 2.698* | C00 | 46.2 | |
| UDF2 | 15639 | 2.696* | C00 | 45.9 | |
| UDF3* | 15876 | 2.543 | LF17 | 98.9 | |
| UDF4 | 15844 | 2.43 | C00 | 42.7 | |
| UDF5 | 13508 | 1.759 | CF00 | 41.7 | LF17/C00 |
| UDF7* | 15381 | 2.59 | C00 | 25.9 | |
| UDF10 | 12743 | 2.086** | CF00 | 18.3 | LF17 |
| UDF11* | 12624 | 1.996 | CF00 | 34.2 | LF17/C00 |
| UDF13* | 15432 | 2.497 | C00 | 20.4 | LF17 |
| UDF15 | 15015 | 1.721** | C00 | 29.0 | LF17 |
Notes. Column 1: target name, sources with an X-ray detection are indicated with a star. Column 2: CANDELS identifier from Guo et al. (2013). Column 3: redshifts from Elbaz et al. (2018) except for sources with one or two stars after the redshift value (from Rujopakarn et al. 2019 and Dunlop et al. 2017 respectively). Columns 4 and 5: best attenuation law (Col. 4) from the best χ2 (Col. 5). Column 6: other attenuation law(s) corresponding to ΔBIC lower than 6 as compared to the best case (ordered by increasing ΔBIC).
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