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LEDA 1069761

Observation

Spectrum ID4585382_sp1
Alt nameg2108089-033303
z0.0679
RA, Dec317.0369, -3.5509
MJD60450.8
SNR/Å B/R9.7/17.0
Obs Airmass1.13
SMSS ID4585382
Closest SMSS11.81'', 4585383
SMSS Mean r6"ap16.1 ± 0.0
2MASS Kext12.4 ± 0.1

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.064
Power law αν-1.16 ± 0.06
log L5100,AGN43.60 ± 0.02
log HβBr/[O III]-0.07 ± 0.02
log ML5100/M7.27 ± 0.05
log M/M7.22 ± 0.03
log M/M7.26 ± 0.05
log M[O III]/M7.45 ± 0.05

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 Narrow40.14 ± 0.37418 ± 63464 ± 261.55 ± 0.78
Hγ Broad41.25 ± 0.062091 ± 468954 ± 8320.12 ± 1.21
[O III] 436439.98 ± 0.26345 ± 63146 ± 251.08 ± 0.40
He II Narrow40.11 ± 0.16345 ± 63146 ± 251.53 ± 0.37
He II Broad41.54 ± 0.0517659 ± 637499 ± 2541.61 ± 2.85
Hβ Narrow40.83 ± 0.10418 ± 63464 ± 268.33 ± 0.75
Hβ Broad41.75 ± 0.021861 ± 991255 ± 5070.21 ± 1.52
[O III] 500741.82 ± 0.01418 ± 63464 ± 2684.10 ± 0.83
He I Narrow40.03 ± 0.12345 ± 63146 ± 251.56 ± 0.25
He I Broad40.78 ± 0.062447 ± 1681039 ± 718.74 ± 0.67
[O I] 630040.31 ± 0.05345 ± 63146 ± 253.11 ± 0.24
Hα Narrow41.18 ± 0.02345 ± 63146 ± 2524.15 ± 0.33
Hα Broad42.27 ± 0.011892 ± 64912 ± 25296.57 ± 1.29
[N II] 658540.96 ± 0.02345 ± 63146 ± 2514.55 ± 0.30
[S II] 671840.73 ± 0.02345 ± 63146 ± 258.68 ± 0.31
[S II] 673240.80 ± 0.02345 ± 63146 ± 2510.22 ± 0.34

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 SNR28.37
Hβ Broad SNR9.94
Hγ Broad SNR3.95
AGN frac0.72
Host frac0.28
log L5100,Host43.19
Fe II/Hβ0.38
Fe II/[O III]0.32

Quality flags

spurious_hab/hbb0.0/0
l51000
balmer0
balmer_snr0
hb_width1
balmer_width1

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