| Spectrum ID | 1030139805_sp1 |
|---|---|
| Alt name | g0401025-004304 |
| z | 0.0139 |
| RA, Dec | 60.2605, -0.7177 |
| MJD | 60260.59 |
| SNR/Å B/R | 4.3/9.0 |
| Obs Airmass | 1.18 |
| SMSS ID | 1030139805 |
| Closest SMSS | 13.10'', 2044938983 |
| SMSS Mean r6"ap | 17.6 ± 0.2 |
| 2MASS Kext | 10.5 ± 0.1 |
| Spectrum Type | Bad |
|---|---|
| Quality Flag | bad_blue |
| AGN reference | 6dFGS |
| MW E(B−V) | 0.415 |
| Power law αν | 0.48 ± 0.02 |
| log L5100,AGN | 41.85 ± 0.01 |
| 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 | 38.60 ± 0.29 | 257 ± 65 | 140 ± 29 | 1.96 ± 0.92 |
| Hγ Broad | — | — | — | — |
| [O III] 4364 | 38.37 ± 0.30 | 219 ± 62 | 93 ± 25 | 1.14 ± 0.64 |
| He II Narrow | — | — | — | — |
| He II Broad | — | — | — | — |
| Hβ Narrow | 38.43 ± 0.30 | 257 ± 65 | 140 ± 29 | 1.72 ± 0.81 |
| Hβ Broad | — | — | — | — |
| [O III] 5007 | 39.30 ± 0.04 | 257 ± 65 | 140 ± 29 | 13.68 ± 0.83 |
| He I Narrow | — | — | — | — |
| He I Broad | — | — | — | — |
| [O I] 6300 | 38.33 ± 0.28 | 219 ± 62 | 93 ± 25 | 2.61 ± 0.94 |
| Hα Narrow | 39.11 ± 0.05 | 219 ± 62 | 93 ± 25 | 17.50 ± 0.85 |
| Hα Broad | — | — | — | — |
| [N II] 6585 | 39.27 ± 0.03 | 219 ± 62 | 93 ± 25 | 25.04 ± 0.83 |
| [S II] 6718 | 38.82 ± 0.07 | 219 ± 62 | 93 ± 25 | 9.47 ± 0.86 |
| [S II] 6732 | 38.84 ± 0.06 | 219 ± 62 | 93 ± 25 | 9.88 ± 1.16 |
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 | 0.78 |
|---|---|
| Hβ Broad SNR | 0.00 |
| Hγ Broad SNR | 0.00 |
| AGN frac | 0.63 |
| Host frac | 0.37 |
| log L5100,Host | 41.61 |
| Fe II/Hβ | — |
| Fe II/[O III] | — |
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.