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LEDA 3904185

Observation

Spectrum ID476888663_sp1
Alt nameg1906088-485027
z0.0488
RA, Dec286.5364, -48.8409
MJD59078.45
SNR/Å B/R7.1/15.1
Obs Airmass1.06
SMSS ID476888663
Closest SMSS13.63'', 476888664
SMSS Mean r6"ap15.9 ± 0.0
2MASS Kext11.3 ± 0.1

AGN Properties

Spectrum TypeSy 1.2
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.061
Power law αν-1.68 ± 0.15
log L5100,AGN42.45 ± 0.05
log HβBr/[O III]0.56 ± 0.04
log ML5100/M7.67 ± 0.07
log M/M7.12 ± 0.03
log M/M7.85 ± 0.07
log M[O III]/M7.71 ± 0.08

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 Narrow39.47 ± 0.40491 ± 79515 ± 315.06 ± 3.37
Hγ Broad40.28 ± 0.133174 ± 7351036 ± 6332.26 ± 4.20
[O III] 436439.16 ± 0.42354 ± 63149 ± 252.48 ± 1.67
He II Narrow39.40 ± 0.23354 ± 63149 ± 254.42 ± 1.55
He II Broad40.34 ± 0.147783 ± 653305 ± 2638.12 ± 6.96
Hβ Narrow40.06 ± 0.15491 ± 79515 ± 3119.68 ± 2.94
Hβ Broad41.07 ± 0.035214 ± 3541998 ± 33207.87 ± 6.01
[O III] 500740.51 ± 0.03491 ± 79515 ± 3158.69 ± 3.03
He I Narrow39.08 ± 0.24354 ± 63149 ± 252.26 ± 0.77
He I Broad40.44 ± 0.066677 ± 642836 ± 2652.19 ± 3.80
[O I] 630039.02 ± 0.26354 ± 63149 ± 252.02 ± 0.75
Hα Narrow40.05 ± 0.04354 ± 63149 ± 2522.19 ± 1.07
Hα Broad41.40 ± 0.013096 ± 811302 ± 25496.41 ± 3.16
[N II] 658540.03 ± 0.04354 ± 63149 ± 2521.04 ± 1.01
[S II] 671839.67 ± 0.07354 ± 63149 ± 259.13 ± 0.82
[S II] 673239.65 ± 0.07354 ± 63149 ± 258.76 ± 0.87

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 SNR9.52
Hβ Broad SNR3.85
Hγ Broad SNR1.38
AGN frac0.26
Host frac0.74
log L5100,Host42.91
Fe II/Hβ0.92
Fe II/[O III]3.28

Quality flags

spurious_hab/hbb0.0/0
l51001
balmer0
balmer_snr1
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.