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LEDA 3095669

Observation

Spectrum ID21947081_sp1
Alt nameg0409135-112502
z0.0914
RA, Dec62.3064, -11.4173
MJD60258.63
SNR/Å B/R14.3/16.6
Obs Airmass1.06
SMSS ID21947081
Closest SMSSNone (< 15")
SMSS Mean r6"ap15.7 ± 0.2
2MASS Kext12.5 ± 0.1

AGN Properties

Spectrum TypeSy 1.2
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.054
Power law αν-0.49 ± 0.02
log L5100,AGN44.36 ± 0.01
log HβBr/[O III]0.57 ± 0.01
log ML5100/M8.15 ± 0.02
log M/M8.08 ± 0.05
log M/M8.27 ± 0.02
log M[O III]/M8.19 ± 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 Narrow40.57 ± 0.29307 ± 63290 ± 270.66 ± 0.39
Hγ Broad42.64 ± 0.023726 ± 1973708 ± 5576.58 ± 1.39
[O III] 436440.58 ± 0.21287 ± 63121 ± 250.67 ± 0.20
He II Narrow40.64 ± 0.15287 ± 63121 ± 250.85 ± 0.19
He II Broad42.35 ± 0.0312949 ± 635499 ± 2543.44 ± 1.35
Hβ Narrow41.06 ± 0.10307 ± 63290 ± 272.36 ± 0.42
Hβ Broad42.78 ± 0.013496 ± 822107 ± 34125.48 ± 1.15
[O III] 500742.21 ± 0.01307 ± 63291 ± 2735.31 ± 0.45
He I Narrow39.94 ± 0.35287 ± 63121 ± 250.24 ± 0.14
He I Broad41.70 ± 0.033645 ± 731548 ± 3013.78 ± 0.57
[O I] 630040.26 ± 0.21287 ± 63121 ± 250.56 ± 0.19
Hα Narrow41.56 ± 0.02287 ± 63121 ± 2511.75 ± 0.32
Hα Broad43.11 ± 0.012805 ± 651427 ± 25420.29 ± 1.03
[N II] 658541.37 ± 0.03287 ± 63121 ± 257.72 ± 0.32
[S II] 671840.99 ± 0.04287 ± 63121 ± 253.28 ± 0.23
[S II] 673240.93 ± 0.04287 ± 63121 ± 252.88 ± 0.22

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 SNR37.97
Hβ Broad SNR17.54
Hγ Broad SNR10.09
AGN frac1.00
Host frac0.00
log L5100,Host41.77
Fe II/Hβ0.37
Fe II/[O III]1.36

Quality flags

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