Table 2.
Measured UV slope and fluxes of emission lines of GELDA stacked spectrum are in erg/cm2/s/Å.
| Parameter | Value |
|---|---|
| flux CIII λ1907 Å | <7.956e-20 |
| flux CIII λ1909 Å | <7.956e-20 |
| flux OII λ3727 Å | <6.105e-21 |
| flux OII λ3730 Å | <6.105e-21 |
| flux OIII λ4960 Å | 7.977E-20 ± 1.039e-20 |
| flux OIII λ5008 Å | 2.559E-19 ± 1.039e-20 |
| flux Hβ (measured) | 4.850E-20 ± 1.039e-20 |
| flux Hβ (2.5% abs.) | 4.971e-20 ± 1.039e-20 |
| flux Hα | 1.422E-19 ± 9.771e-21 |
| flux NII λ6550 Å | <9.771e-21 |
| flux NII λ6585 Å | <9.771e-21 |
| βFUV | –2.451 ± 0.066 |
| RH(F200W) | 380 ± 132 pc |
| MFUV | –18.9 ± 0.9 |
| log10(Mstar) | 8.36 ± 0.37 |
Notes. We corrected the Hβ flux for the underlying absorption that increases Hβ by 2.5%, but we did not correct for Hα, which is assumed negligible (Kashino et al. 2013; Reddy et al. 2015; Shivaei et al. 2020). With this underlying absorption, we conclude there is no dust attenuation for Case B for these GELDAs.
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