MCG-01-22-028
Observation
| Spectrum ID | 75454716_sp1 |
|---|---|
| Alt name | MCG -1-22-028 |
| z | 0.0363 |
| RA, Dec | 129.0388, -7.0549 |
| MJD | 61009.7 |
| SNR/Å B/R | 20.6/42.4 |
| Obs Airmass | 1.16 |
| SMSS ID | 75454716 |
| Closest SMSS | 8.24'', 2113993222 |
| SMSS Mean r6"ap | 14.7 ± 0.0 |
| 2MASS Kext | 10.2 ± 0.0 |
AGN Properties
| Spectrum Type | SF |
|---|---|
| Quality Flag | good |
| AGN reference | PGC |
| MW E(B−V) | 0.030 |
| Power law αν | 0.49 ± 0.01 |
| log L5100,AGN | 42.03 ± 0.21 |
| log HβBr/[O III] | — |
| log ML5100/M☉ | — |
| log MHα/M☉ | — |
| log MHβ/M☉ | — |
| log M[O III]/M☉ | — |
Spatial extraction & sky subtraction region
Spaxel scale: 1 arcsec² — Flux units: erg s⁻¹ cm⁻² Å⁻¹
Apertures: object (solid), background (dashed)
Spectrum decomposition
Emission line measurements
| 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 | 40.33 ± 0.12 | 3021 ± 62 | 1283 ± 25 | 84.03 ± 12.50 |
| Hβ Narrow | — | — | — | — |
| Hβ Broad | — | — | — | — |
| [O III] 5007 | 40.18 ± 0.09 | 1190 ± 471 | 529 ± 25 | 68.84 ± 8.41 |
| He I Narrow | — | — | — | — |
| He I Broad | — | — | — | — |
| [O I] 6300 | — | — | — | — |
| Hα Narrow | 39.92 ± 0.05 | 305 ± 62 | 129 ± 25 | 75.31 ± 5.44 |
| Hα Broad | — | — | — | — |
| [N II] 6585 | 40.21 ± 0.03 | 305 ± 62 | 129 ± 25 | 145.99 ± 6.12 |
| [S II] 6718 | 39.79 ± 0.07 | 305 ± 62 | 129 ± 25 | 58.77 ± 5.93 |
| [S II] 6732 | 39.74 ± 0.08 | 305 ± 62 | 129 ± 25 | 52.85 ± 6.11 |
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.
Emission summary
| Hα Broad SNR | 0.80 |
|---|---|
| Hβ Broad SNR | 0.00 |
| Hγ Broad SNR | 0.00 |
| AGN frac | 0.02 |
| Host frac | 0.98 |
| log L5100,Host | 43.64 |
| Fe II/Hβ | — |
| Fe II/[O III] | 6.91 |
Quality flags
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.