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2MASS J21450570-6922309

Observation

Spectrum ID486517428_sp1
Alt nameg2145058-692231
z0.0891
RA, Dec326.2738, -69.3752
MJD60086.8
SNR/Å B/R9.1/10.0
Obs Airmass1.27
SMSS ID486517428
Closest SMSS12.83'', 486517398
SMSS Mean r6"ap16.7 ± 0.1
2MASS Kext13.1 ± 0.1

AGN Properties

Spectrum TypeSy 1.2
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.030
Power law αν-0.78 ± 0.08
log L5100,AGN43.82 ± 0.02
log HβBr/[O III]0.49 ± 0.04
log ML5100/M7.40 ± 0.11
log M/M7.09 ± 0.11
log M/M7.34 ± 0.11
log M[O III]/M7.26 ± 0.11

Spatial extraction & sky subtraction region

Spatial plot

Spaxel scale: 1 arcsec² — Flux units: erg s⁻¹ cm⁻² Å⁻¹
Apertures: object (solid), background (dashed)

Spectrum decomposition

Emission line measurements

Linelog L (erg s⁻¹)FWHM (km s⁻¹)σ (km s⁻¹)EW (Å)
Hγ Narrow40.58 ± 0.19473 ± 83201 ± 342.42 ± 0.39
Hγ Broad41.33 ± 0.061235 ± 72469 ± 2613.07 ± 0.64
[O III] 436440.19 ± 0.26473 ± 83200 ± 351.02 ± 0.37
He II Narrow40.22 ± 0.31473 ± 83200 ± 351.22 ± 0.36
He II Broad40.75 ± 0.161235 ± 72524 ± 293.88 ± 0.59
Hβ Narrow41.21 ± 0.11473 ± 83201 ± 3411.43 ± 0.42
Hβ Broad41.85 ± 0.021940 ± 235862 ± 4251.32 ± 0.99
[O III] 500741.36 ± 0.03473 ± 83201 ± 3417.43 ± 0.45
He I Narrow39.97 ± 0.35473 ± 83200 ± 350.91 ± 0.38
He I Broad40.66 ± 0.131193 ± 65506 ± 264.15 ± 0.58
[O I] 630039.97 ± 0.28473 ± 83200 ± 350.97 ± 0.41
Hα Narrow41.75 ± 0.10473 ± 83200 ± 3559.27 ± 0.51
Hα Broad42.29 ± 0.031590 ± 196662 ± 29206.78 ± 1.02
[N II] 658540.98 ± 0.07473 ± 83200 ± 3510.39 ± 0.48
[S II] 671840.53 ± 0.11473 ± 83200 ± 353.86 ± 0.54
[S II] 673240.24 ± 0.17473 ± 83200 ± 351.97 ± 0.56

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 SNR24.83
Hβ Broad SNR9.51
Hγ Broad SNR5.62
AGN frac0.95
Host frac0.05
log L5100,Host42.53
Fe II/Hβ1.69
Fe II/[O III]5.16

Quality flags

spurious_hab/hbb0.0/0
l51000
balmer0
balmer_snr0
hb_width0
balmer_width0

Hα mass estimates from Cho+2023. Remaining mass estimates from R–L relations in Wang & Woo 2024 and zero-points from Amrutha+2026.