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LEDA 3096589

Observation

Spectrum ID234143384_sp1
Alt nameg2039272-301852
z0.0796
RA, Dec309.8633, -30.3145
MJD60082.74
SNR/Å B/R16.5/20.7
Obs Airmass1.04
SMSS ID234143384
Closest SMSS13.96'', 234143625
SMSS Mean r6"ap15.8 ± 0.1
2MASS Kextnan ± nan

AGN Properties

Spectrum TypeSy 1.2
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.060
Power law αν-0.69 ± 0.07
log L5100,AGN44.08 ± 0.01
log HβBr/[O III]0.32 ± 0.01
log ML5100/M7.30 ± 0.03
log M/M7.22 ± 0.05
log M/M7.30 ± 0.03
log M[O III]/M7.32 ± 0.03

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 Narrow41.04 ± 0.10481 ± 63398 ± 263.77 ± 0.34
Hγ Broad41.62 ± 0.041271 ± 70646 ± 5114.31 ± 0.56
[O III] 436439.75 ± 0.43461 ± 63195 ± 250.20 ± 0.20
He II Narrow40.40 ± 0.17461 ± 63195 ± 250.96 ± 0.21
He II Broad41.13 ± 0.093568 ± 1291515 ± 545.15 ± 0.58
Hβ Narrow41.53 ± 0.04481 ± 63398 ± 2613.48 ± 0.37
Hβ Broad42.23 ± 0.011512 ± 521087 ± 3168.30 ± 0.75
[O III] 500741.92 ± 0.01481 ± 63398 ± 2634.53 ± 0.40
He I Narrow39.98 ± 0.29461 ± 63195 ± 250.49 ± 0.18
He I Broad41.22 ± 0.042105 ± 86894 ± 358.71 ± 0.44
[O I] 630040.51 ± 0.07461 ± 63195 ± 251.85 ± 0.19
Hα Narrow41.93 ± 0.01461 ± 63195 ± 2551.00 ± 0.37
Hα Broad42.70 ± 0.011389 ± 63709 ± 25301.74 ± 0.71
[N II] 658541.22 ± 0.03461 ± 63195 ± 259.92 ± 0.31
[S II] 671840.63 ± 0.07461 ± 63195 ± 252.60 ± 0.29
[S II] 673240.53 ± 0.08461 ± 63195 ± 252.10 ± 0.29

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 SNR63.02
Hβ Broad SNR22.12
Hγ Broad SNR8.39
AGN frac0.92
Host frac0.08
log L5100,Host42.99
Fe II/Hβ1.54
Fe II/[O III]3.17

Quality flags

spurious_hab/hbb0.0/0
l51000
balmer0
balmer_snr0
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.