| Spectrum ID | 103884059_sp1 |
|---|---|
| Alt name | ISZ 96 |
| z | 0.0624 |
| RA, Dec | 180.1810, -20.8337 |
| MJD | 61068.74 |
| SNR/Å B/R | 17.3/28.6 |
| Obs Airmass | 1.02 |
| SMSS ID | 103884059 |
| Closest SMSS | 8.75'', 103884060 |
| SMSS Mean r6"ap | 15.5 ± 0.0 |
| 2MASS Kext | 11.5 ± 0.1 |
| Spectrum Type | Sy 2 |
|---|---|
| Quality Flag | good |
| AGN reference | PGC |
| MW E(B−V) | 0.044 |
| Power law αν | 0.30 ± 0.11 |
| log L5100,AGN | 43.60 ± 0.02 |
| 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 | 39.95 ± 0.30 | 646 ± 62 | 274 ± 25 | 0.79 ± 0.36 |
| He II Narrow | 40.41 ± 0.11 | 646 ± 62 | 274 ± 25 | 2.69 ± 0.39 |
| He II Broad | 41.38 ± 0.07 | 15483 ± 62 | 6575 ± 25 | 25.52 ± 1.98 |
| Hβ Narrow | 40.72 ± 0.10 | 690 ± 63 | 408 ± 26 | 6.05 ± 0.60 |
| Hβ Broad | — | — | — | — |
| [O III] 5007 | 41.91 ± 0.01 | 690 ± 63 | 408 ± 26 | 99.20 ± 0.72 |
| He I Narrow | 40.01 ± 0.17 | 646 ± 62 | 274 ± 25 | 1.82 ± 0.40 |
| He I Broad | — | — | — | — |
| [O I] 6300 | 40.47 ± 0.05 | 646 ± 62 | 274 ± 25 | 6.07 ± 0.45 |
| Hα Narrow | 41.88 ± 0.01 | 646 ± 62 | 274 ± 25 | 122.31 ± 0.69 |
| Hα Broad | — | — | — | — |
| [N II] 6585 | 41.63 ± 0.01 | 646 ± 62 | 274 ± 25 | 68.81 ± 0.68 |
| [S II] 6718 | 41.05 ± 0.02 | 646 ± 62 | 274 ± 25 | 26.90 ± 0.59 |
| [S II] 6732 | 41.20 ± 0.01 | 646 ± 62 | 274 ± 25 | 38.24 ± 0.60 |
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 | 0.00 |
|---|---|
| Hβ Broad SNR | 0.00 |
| Hγ Broad SNR | 0.00 |
| AGN frac | 0.42 |
| Host frac | 0.58 |
| log L5100,Host | 43.74 |
| Fe II/Hβ | — |
| Fe II/[O III] | 0.17 |
spurious_hab/hbb | 1.0/0 |
|---|---|
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.