| Spectrum ID | 21832881_sp1 |
|---|---|
| Alt name | g0339579-061215 |
| z | 0.0501 |
| RA, Dec | 54.9912, -6.2042 |
| MJD | 60914.79 |
| SNR/Å B/R | 9.6/20.7 |
| Obs Airmass | 1.11 |
| SMSS ID | 21832881 |
| Closest SMSS | 14.61'', 21832880 |
| SMSS Mean r6"ap | 16.6 ± 0.1 |
| 2MASS Kext | 12.1 ± 0.1 |
| Spectrum Type | Sy 2 |
|---|---|
| Quality Flag | good |
| AGN reference | 6dFGS |
| MW E(B−V) | 0.043 |
| Power law αν | -1.96 ± 0.04 |
| log L5100,AGN | 41.81 ± 0.22 |
| log HβBr/[O III] | — |
| log ML5100/M☉ | — |
| log MHα/M☉ | — |
| 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 | 38.97 ± 0.40 | 267 ± 62 | 112 ± 25 | 7.32 ± 5.88 |
| He II Broad | 40.42 ± 0.13 | 6034 ± 62 | 2562 ± 25 | 204.69 ± 30.32 |
| Hβ Narrow | 39.47 ± 0.33 | 348 ± 91 | 522 ± 44 | 21.63 ± 12.76 |
| Hβ Broad | — | — | — | — |
| [O III] 5007 | 39.92 ± 0.13 | 348 ± 91 | 522 ± 44 | 65.91 ± 12.60 |
| He I Narrow | 38.83 ± 0.38 | 267 ± 62 | 112 ± 25 | 5.33 ± 3.23 |
| He I Broad | 39.55 ± 0.28 | 2349 ± 62 | 998 ± 25 | 28.44 ± 9.80 |
| [O I] 6300 | — | — | — | — |
| Hα Narrow | 39.92 ± 0.05 | 267 ± 62 | 112 ± 25 | 65.64 ± 3.95 |
| Hα Broad | — | — | — | — |
| [N II] 6585 | 39.92 ± 0.04 | 267 ± 62 | 112 ± 25 | 65.83 ± 3.86 |
| [S II] 6718 | 39.57 ± 0.09 | 267 ± 62 | 112 ± 25 | 29.59 ± 3.32 |
| [S II] 6732 | 39.34 ± 0.14 | 267 ± 62 | 112 ± 25 | 17.65 ± 3.24 |
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 | 0.92 |
|---|---|
| Hβ Broad SNR | 0.00 |
| Hγ Broad SNR | 0.00 |
| AGN frac | 0.04 |
| Host frac | 0.96 |
| log L5100,Host | 43.20 |
| Fe II/Hβ | — |
| Fe II/[O III] | 1.55 |
spurious_hab/hbb | 0.0/0 |
|---|---|
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.