Table 2.
Best-fit emission line properties from JWST/NIRCam F410M grism spectra, and best-fit UV and optical slopes from photometric bands.
| ID | zspec | FluxHβ, broad | FluxHβ, narrow | Flux[O III]λ5008 | FWHMHβ,broad | FWHMnarrow | βUV | βopt |
|---|---|---|---|---|---|---|---|---|
| 10−18 erg s−1 cm−2 | 10−18 erg s−1 cm−2 | 10−18 erg s−1 cm−2 | km s−1 | km s−1 | ||||
| ID9094 | 7.0388 ± 0.0001 | 6.95 ± 1.57 | 2.01 ± 0.63 | 24.47 ± 0.49 | 2280 ± 490 | 425 ± 10 | −1.05 ± 0.24 | 1.14 ± 0.31 |
| ID2756 | 7.1883 ± 0.0001 | 2.65 ± 0.65 | 0.52 ± 0.40 | 6.69 ± 0.29 | 1070 ± 240 | 295 ± 16 | −1.48 ± 0.12 | 0.26 ± 0.31 |
Notes.βUV and βopt are continuum slopes derived from multi-band JWST photometry blueward and redward of the Balmer break, respectively, and trace the two sides of the “v-shaped” SEDs (see Sect. 2.4).
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