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LEDA 3098145

Observation

Spectrum ID307031075_sp1
Alt nameg1514487-402153
z0.0238
RA, Dec228.7029, -40.3648
MJD59078.36
SNR/Å B/R21.1/45.2
Obs Airmass1.04
SMSS ID307031075
Closest SMSS13.77'', 307031145
SMSS Mean r6"ap14.9 ± 0.0
2MASS Kext10.8 ± 0.0

AGN Properties

Spectrum TypeSy 1.2
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.094
Power law αν0.19 ± 0.24
log L5100,AGN42.31 ± 0.04
log HβBr/[O III]0.67 ± 0.02
log ML5100/M7.36 ± 0.05
log M/M7.28 ± 0.03
log M/M7.61 ± 0.05
log M[O III]/M7.42 ± 0.06

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 Narrow38.78 ± 0.46405 ± 65157 ± 251.06 ± 1.00
Hγ Broad39.95 ± 0.142018 ± 648917 ± 7415.04 ± 3.04
[O III] 436439.14 ± 0.25256 ± 63108 ± 252.50 ± 0.91
He II Narrow38.97 ± 0.28256 ± 63108 ± 251.96 ± 0.85
He II Broad40.34 ± 0.099091 ± 723861 ± 2945.45 ± 5.12
Hβ Narrow39.11 ± 0.27405 ± 65157 ± 252.90 ± 0.96
Hβ Broad41.10 ± 0.023897 ± 1253958 ± 94289.55 ± 7.51
[O III] 500740.43 ± 0.01405 ± 65157 ± 2565.66 ± 1.06
He I Narrow38.33 ± 0.42256 ± 63108 ± 250.74 ± 0.69
He I Broad40.29 ± 0.044979 ± 692114 ± 2866.80 ± 3.71
[O I] 630038.58 ± 0.33256 ± 63108 ± 251.52 ± 0.82
Hα Narrow39.76 ± 0.03256 ± 63108 ± 2525.19 ± 1.01
Hα Broad41.44 ± 0.013606 ± 651495 ± 301201.76 ± 5.43
[N II] 658539.96 ± 0.02256 ± 63108 ± 2540.68 ± 1.03
[S II] 671839.34 ± 0.08256 ± 63108 ± 2510.17 ± 1.19
[S II] 673239.26 ± 0.09256 ± 63108 ± 258.37 ± 1.10

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 SNR14.96
Hβ Broad SNR5.46
Hγ Broad SNR1.37
AGN frac0.10
Host frac0.90
log L5100,Host43.27
Fe II/Hβ0.59
Fe II/[O III]2.76

Quality flags

spurious_hab/hbb0.0/0
l51002
balmer0
balmer_snr1
hb_width2
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.