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Table B.1.

Overview of model fits to the Hβ and Hα profiles in optical spectra.

Spec. Time Telescope Hβ-λ range Hα-λ range [O III]-model Broad Hβ-model
- 53408 6dF (4600 Å, 5160 Å) (6416 Å, 6760 Å) 1-Gaussian 2-Gaussian
S1 58871 Keck (4500 Å, 5160 Å) (6200 Å, 6900 Å) 3-Gaussian 2-Gaussian
S2 58905 LDT (4500 Å, 5160 Å) (6300 Å, 6800 Å) 3-Gaussian 2-Gaussian
S3 59105 LDT (4500 Å, 5160 Å) (6300 Å, 6800 Å) 2-Gaussian 2-Gaussian
S4 59189 LDT (4500 Å, 5160 Å) (6300 Å, 6800 Å) 2-Gaussian 2-Gaussian
S5 59468 SAAO (4500 Å, 5160 Å) (6300 Å, 6800 Å) 2-Gaussian 1-Gaussian
S6 59586 SALT (4500 Å, 5160 Å) (6300 Å, 6760 Å) 2-Gaussian 1-Gaussian
S7 59660 FORS2 (4500 Å, 5160 Å) (6300 Å, 6800 Å) 2-Gaussian 2-Gaussian
S8 59828 DBSP (4500 Å, 5160 Å) (6300 Å, 6800 Å) 2-Gaussian 1-Gaussian
S9 59881 SALT (4500 Å, 5160 Å) (6300 Å, 6800 Å) 2-Gaussian 2-Gaussian
S10 59883 SALT (4500 Å, 5160 Å) (6300Å, 6800Å) 2-Gaussian 1-Gaussian
S11 60018 FORS2 (4500 Å, 5160 Å) (6300Å, 6800Å) 2-Gaussian 2-Gaussian

Notes. Columns 4 and 5 list the wavelength ranges used for local fitting of the broad Balmer profiles line regions. Columns 6 and 7 lists the (signal-to-noise-dependent) model used for fitting the [O III] λλ4959,5007 and Hβ profiles, respectively.

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