| Spectrum ID | 306475963_sp1 |
|---|---|
| Alt name | g1439442-394242 |
| z | 0.0840 |
| RA, Dec | 219.9339, -39.7115 |
| MJD | 60378.73 |
| SNR/Å B/R | 18.3/27.0 |
| Obs Airmass | 1.01 |
| SMSS ID | 306475963 |
| Closest SMSS | 9.83'', 306475962 |
| SMSS Mean r6"ap | 16.6 ± 0.1 |
| 2MASS Kext | 12.5 ± 0.1 |
| Spectrum Type | Sy 1.5+ |
|---|---|
| Quality Flag | good |
| AGN reference | 6dFGS |
| MW E(B−V) | 0.081 |
| Power law αν | -1.69 ± 0.13 |
| log L5100,AGN | 42.77 ± 0.07 |
| log HβBr/[O III] | <0.30 |
| log ML5100/M☉ | — |
| log MHα/M☉ | 8.10 ± 0.07 |
| log MHβ/M☉ | — |
| log M[O III]/M☉ | — |

Spaxel scale: 1 arcsec² — Flux units: erg s⁻¹ cm⁻² Å⁻¹
Apertures: object (solid), background (dashed)
| Line | log L (erg s⁻¹) | FWHM (km s⁻¹) | σ (km s⁻¹) | EW (Å) |
|---|---|---|---|---|
| Hγ Narrow | — | — | — | — |
| Hγ Broad | — | — | — | — |
| [O III] 4364 | — | — | — | — |
| He II Narrow | — | — | — | — |
| He II Broad | — | — | — | — |
| Hβ Narrow | — | — | — | — |
| Hβ Broad | <40.96 | — | — | — |
| [O III] 5007 | 40.66 ± 0.06 | 344 ± 63 | 343 ± 84 | 39.63 ± 3.25 |
| He I Narrow | — | — | — | — |
| He I Broad | 40.09 ± 0.28 | 3004 ± 62 | 1276 ± 25 | 11.16 ± 3.97 |
| [O I] 6300 | 39.87 ± 0.16 | 330 ± 62 | 140 ± 25 | 6.97 ± 1.35 |
| Hα Narrow | 40.34 ± 0.05 | 330 ± 62 | 140 ± 25 | 20.61 ± 1.26 |
| Hα Broad | 41.42 ± 0.03 | 9399 ± 636 | 3565 ± 32 | 249.88 ± 8.92 |
| [N II] 6585 | 40.58 ± 0.03 | 330 ± 62 | 140 ± 25 | 36.05 ± 1.37 |
| [S II] 6718 | 40.01 ± 0.13 | 330 ± 62 | 140 ± 25 | 9.68 ± 1.89 |
| [S II] 6732 | 40.16 ± 0.08 | 330 ± 62 | 140 ± 25 | 13.69 ± 1.67 |
All narrow line widths are tied to narrow [O III] 5007Å. [O III] 5007Å and narrow Hβ include a second narrow component not tied to other narrow lines.
| Hα Broad SNR | 1.51 |
|---|---|
| Hβ Broad SNR | 0.00 |
| Hγ Broad SNR | 0.00 |
| AGN frac | 0.09 |
| Host frac | 0.91 |
| log L5100,Host | 43.78 |
| Fe II/Hβ | — |
| Fe II/[O III] | — |
spurious_hab/hbb | 0.0/1 |
|---|---|
l5100 | 2 |
balmer | 2 |
balmer_snr | 2 |
hb_width | 2 |
balmer_width | 2 |
Hα mass estimates from Cho+2023. Remaining mass estimates from R–L relations in Wang & Woo 2024 and zero-points from Amrutha+2026.