| Spectrum ID | 17832134_sp1 |
|---|---|
| Alt name | g0321104-212929 |
| z | 0.0722 |
| RA, Dec | 50.2932, -21.4914 |
| MJD | 60258.52 |
| SNR/Å B/R | 11.9/21.7 |
| Obs Airmass | 1.09 |
| SMSS ID | 17832134 |
| Closest SMSS | None (< 15") |
| SMSS Mean r6"ap | 16.9 ± 0.1 |
| 2MASS Kext | 12.5 ± 0.1 |
| Spectrum Type | Sy 1.5+ |
|---|---|
| Quality Flag | good |
| AGN reference | 6dFGS |
| MW E(B−V) | 0.021 |
| Power law αν | -0.33 ± 0.15 |
| log L5100,AGN | 42.94 ± 0.03 |
| log HβBr/[O III] | <-0.29 |
| log ML5100/M☉ | — |
| log MHα/M☉ | 7.00 ± 0.05 |
| 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 | 39.20 ± 0.44 | 252 ± 62 | 106 ± 25 | 0.80 ± 0.60 |
| He II Broad | — | — | — | — |
| Hβ Narrow | 39.70 ± 0.21 | 257 ± 63 | 311 ± 45 | 2.66 ± 1.47 |
| Hβ Broad | <40.57 | — | — | — |
| [O III] 5007 | 40.86 ± 0.03 | 257 ± 63 | 311 ± 45 | 41.16 ± 1.72 |
| He I Narrow | — | — | — | — |
| He I Broad | — | — | — | — |
| [O I] 6300 | 39.46 ± 0.18 | 252 ± 62 | 106 ± 25 | 2.40 ± 0.58 |
| Hα Narrow | 40.45 ± 0.02 | 252 ± 62 | 106 ± 25 | 24.86 ± 0.69 |
| Hα Broad | 41.23 ± 0.02 | 3036 ± 144 | 1357 ± 37 | 151.60 ± 3.54 |
| [N II] 6585 | 40.57 ± 0.02 | 252 ± 62 | 106 ± 25 | 33.31 ± 0.75 |
| [S II] 6718 | 40.13 ± 0.05 | 252 ± 62 | 106 ± 25 | 12.30 ± 0.78 |
| [S II] 6732 | 40.05 ± 0.05 | 252 ± 62 | 106 ± 25 | 10.42 ± 0.72 |
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 | 3.12 |
|---|---|
| Hβ Broad SNR | 0.27 |
| Hγ Broad SNR | 0.00 |
| AGN frac | 0.24 |
| Host frac | 0.76 |
| log L5100,Host | 43.44 |
| Fe II/Hβ | — |
| Fe II/[O III] | — |
spurious_hab/hbb | 0.0/1 |
|---|---|
l5100 | 1 |
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.