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LEDA 668116

Observation

Spectrum ID19795813_sp1
Alt nameg0529592-340159
z0.0788
RA, Dec82.4967, -34.0329
MJD59668.38
SNR/Å B/R8.6/15.3
Obs Airmass1.11
SMSS ID19795813
Closest SMSS5.13'', 2041549029
SMSS Mean r6"ap16.0 ± 0.1
2MASS Kext12.5 ± 0.2

AGN Properties

Spectrum TypeSy 1.8
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.016
Power law αν-0.70 ± 0.20
log L5100,AGN43.55 ± 0.04
log HβBr/[O III]-0.50 ± 0.07
log ML5100/M8.51 ± 0.24
log M/M8.50 ± 0.02
log M/M8.46 ± 0.24
log M[O III]/M8.86 ± 0.24

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 Narrow40.46 ± 0.31674 ± 62286 ± 253.35 ± 1.03
Hγ Broad40.68 ± 0.271267 ± 100467 ± 414.17 ± 1.46
[O III] 436440.13 ± 0.37673 ± 62285 ± 251.59 ± 0.99
He II Narrow40.32 ± 0.31673 ± 62285 ± 252.70 ± 0.98
He II Broad40.21 ± 0.461216 ± 62516 ± 252.10 ± 1.29
Hβ Narrow41.07 ± 0.07674 ± 62286 ± 2515.94 ± 1.09
Hβ Broad41.63 ± 0.067945 ± 22253752 ± 7855.82 ± 4.33
[O III] 500742.13 ± 0.01674 ± 62286 ± 25187.21 ± 1.33
He I Narrow39.89 ± 0.38673 ± 62285 ± 251.34 ± 0.70
He I Broad40.09 ± 0.411938 ± 62823 ± 252.14 ± 1.37
[O I] 630040.45 ± 0.11673 ± 62285 ± 255.34 ± 0.81
Hα Narrow41.65 ± 0.01673 ± 62285 ± 2589.60 ± 1.06
Hα Broad42.09 ± 0.029282 ± 2313512 ± 34247.75 ± 4.00
[N II] 658541.51 ± 0.01673 ± 62285 ± 2564.89 ± 1.04
[S II] 671841.13 ± 0.04673 ± 62285 ± 2527.96 ± 1.29
[S II] 673240.99 ± 0.04673 ± 62285 ± 2520.18 ± 1.32

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 SNR2.50
Hβ Broad SNR1.32
Hγ Broad SNR1.03
AGN frac0.41
Host frac0.59
log L5100,Host43.71
Fe II/Hβ0.85
Fe II/[O III]0.26

Quality flags

spurious_hab/hbb0.0/0
l51001
balmer1
balmer_snr2
hb_width0
balmer_width2

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