| Spectrum ID | 96500476_sp1 |
|---|---|
| Alt name | g1325194-382453 |
| z | 0.0661 |
| RA, Dec | 201.3307, -38.4146 |
| MJD | 60079.49 |
| SNR/Å B/R | 1.7/1.8 |
| Obs Airmass | 1.01 |
| SMSS ID | 96500476 |
| Closest SMSS | 6.83'', 96500478 |
| SMSS Mean r6"ap | 15.9 ± 0.1 |
| 2MASS Kext | 11.9 ± 0.1 |
| Spectrum Type | Bad |
|---|---|
| Quality Flag | bad_all |
| AGN reference | 6dFGS |
| MW E(B−V) | 0.060 |
| Power law αν | 0.49 ± 0.01 |
| log L5100,AGN | 42.57 ± 0.01 |
| log HβBr/[O III] | 0.45 ± 0.15 |
| log ML5100/M☉ | 7.07 ± 0.19 |
| log MHα/M☉ | 5.76 ± 0.08 |
| log MHβ/M☉ | 6.99 ± 0.20 |
| log M[O III]/M☉ | 6.88 ± 0.21 |

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 | 39.91 ± 0.27 | 191 ± 78 | 573 ± 27 | 7.31 ± 3.04 |
| Hγ Broad | — | — | — | — |
| [O III] 4364 | — | — | — | — |
| He II Narrow | 39.24 ± 0.22 | 126 ± 62 | 51 ± 25 | 1.92 ± 0.90 |
| He II Broad | 39.70 ± 0.35 | 1389 ± 62 | 590 ± 25 | 5.49 ± 3.06 |
| Hβ Narrow | — | — | — | — |
| Hβ Broad | 40.62 ± 0.08 | 2448 ± 585 | 1094 ± 54 | 50.15 ± 5.01 |
| [O III] 5007 | 40.16 ± 0.13 | 191 ± 78 | 573 ± 27 | 18.80 ± 4.46 |
| He I Narrow | — | — | — | — |
| He I Broad | — | — | — | — |
| [O I] 6300 | — | — | — | — |
| Hα Narrow | — | — | — | — |
| Hα Broad | 40.51 ± 0.03 | 1201 ± 66 | 455 ± 31 | 81.86 ± 3.61 |
| [N II] 6585 | — | — | — | — |
| [S II] 6718 | 38.74 ± 0.37 | 126 ± 62 | 51 ± 25 | 1.50 ± 1.07 |
| [S II] 6732 | 39.12 ± 0.20 | 126 ± 62 | 51 ± 25 | 3.56 ± 0.98 |
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 | 2.34 |
|---|---|
| Hβ Broad SNR | 1.86 |
| Hγ Broad SNR | 0.48 |
| AGN frac | 1.00 |
| Host frac | 0.00 |
| log L5100,Host | 39.88 |
| Fe II/Hβ | 1.07 |
| Fe II/[O III] | 3.07 |
spurious_hab/hbb | 0.0/0 |
|---|---|
l5100 | 2 |
balmer | 2 |
balmer_snr | 2 |
hb_width | 0 |
balmer_width | 1 |
Hα mass estimates from Cho+2023. Remaining mass estimates from R–L relations in Wang & Woo 2024 and zero-points from Amrutha+2026.