| Spectrum ID | 488457185_sp1 |
|---|---|
| Alt name | ESO287-G42 |
| z | 0.0186 |
| RA, Dec | 324.5329, -42.6050 |
| MJD | 60911.55 |
| SNR/Å B/R | 28.1/51.9 |
| Obs Airmass | 1.02 |
| SMSS ID | 488457185 |
| Closest SMSS | None (< 15") |
| SMSS Mean r6"ap | nan ± nan |
| 2MASS Kext | 11.1 ± 0.0 |
| Spectrum Type | Sy 1.5+ |
|---|---|
| Quality Flag | good |
| AGN reference | S7 |
| MW E(B−V) | 0.018 |
| Power law αν | -1.98 ± 0.02 |
| log L5100,AGN | 41.61 ± 0.22 |
| log HβBr/[O III] | <-0.09 |
| log ML5100/M☉ | — |
| log MHα/M☉ | 6.73 ± 0.09 |
| 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 | 38.58 ± 0.39 | 406 ± 64 | 393 ± 46 | 4.71 ± 4.28 |
| Hγ Broad | — | — | — | — |
| [O III] 4364 | — | — | — | — |
| He II Narrow | — | — | — | — |
| He II Broad | — | — | — | — |
| Hβ Narrow | 39.42 ± 0.07 | 406 ± 64 | 394 ± 45 | 32.35 ± 3.72 |
| Hβ Broad | <39.59 | — | — | — |
| [O III] 5007 | 39.68 ± 0.04 | 406 ± 64 | 394 ± 45 | 59.87 ± 3.49 |
| He I Narrow | — | — | — | — |
| He I Broad | — | — | — | — |
| [O I] 6300 | 39.05 ± 0.06 | 364 ± 62 | 154 ± 25 | 14.22 ± 1.25 |
| Hα Narrow | 39.80 ± 0.02 | 364 ± 62 | 154 ± 25 | 79.84 ± 1.34 |
| Hα Broad | 40.17 ± 0.03 | 4691 ± 250 | 1891 ± 47 | 183.43 ± 5.12 |
| [N II] 6585 | 39.54 ± 0.02 | 364 ± 62 | 154 ± 25 | 43.28 ± 1.29 |
| [S II] 6718 | 39.58 ± 0.02 | 364 ± 62 | 154 ± 25 | 48.30 ± 1.37 |
| [S II] 6732 | 39.50 ± 0.02 | 364 ± 62 | 154 ± 25 | 39.76 ± 1.45 |
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 | 1.95 |
|---|---|
| Hβ Broad SNR | 0.51 |
| Hγ Broad SNR | 0.00 |
| AGN frac | 0.05 |
| Host frac | 0.95 |
| log L5100,Host | 42.91 |
| Fe II/Hβ | — |
| Fe II/[O III] | — |
spurious_hab/hbb | 0.0/2 |
|---|---|
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.