| Spectrum ID | 78936632_sp2 |
|---|---|
| Alt name | g0919278-312202 |
| z | 0.0370 |
| RA, Dec | 139.8659, -31.3673 |
| MJD | 60351.55 |
| SNR/Å B/R | 9.8/18.8 |
| Obs Airmass | 1.01 |
| SMSS ID | 78936632 |
| Closest SMSS | 8.58'', 78936641 |
| SMSS Mean r6"ap | 16.9 ± 0.1 |
| 2MASS Kext | 11.5 ± 0.1 |
| Spectrum Type | Sy 1.5+ |
|---|---|
| Quality Flag | good |
| AGN reference | 6dFGS |
| MW E(B−V) | 0.161 |
| Power law αν | -1.98 ± 0.02 |
| log L5100,AGN | 40.48 ± 0.71 |
| log HβBr/[O III] | <0.03 |
| log ML5100/M☉ | — |
| log MHα/M☉ | 6.42 ± 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 | 39.21 ± 0.18 | 207 ± 63 | 435 ± 39 | 271.60 ± 131.56 |
| Hβ Broad | <40.05 | — | — | — |
| [O III] 5007 | 40.02 ± 0.06 | 207 ± 63 | 435 ± 39 | 1768.73 ± 140.01 |
| He I Narrow | — | — | — | — |
| He I Broad | 39.55 ± 0.16 | 2108 ± 62 | 895 ± 25 | 596.67 ± 122.08 |
| [O I] 6300 | 38.55 ± 0.33 | 187 ± 62 | 75 ± 25 | 59.76 ± 35.65 |
| Hα Narrow | 39.72 ± 0.03 | 187 ± 62 | 75 ± 25 | 882.77 ± 39.07 |
| Hα Broad | 40.33 ± 0.04 | 2923 ± 63 | 1071 ± 25 | 3587.08 ± 157.63 |
| [N II] 6585 | 39.79 ± 0.03 | 187 ± 62 | 75 ± 25 | 1043.00 ± 42.32 |
| [S II] 6718 | 39.47 ± 0.05 | 187 ± 62 | 75 ± 25 | 494.35 ± 38.59 |
| [S II] 6732 | 39.25 ± 0.08 | 187 ± 62 | 75 ± 25 | 303.94 ± 40.75 |
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 | 1.70 |
|---|---|
| Hβ Broad SNR | 0.80 |
| Hγ Broad SNR | 0.00 |
| AGN frac | 0.00 |
| Host frac | 1.00 |
| log L5100,Host | 42.90 |
| Fe II/Hβ | — |
| Fe II/[O III] | 3.20 |
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.