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LEDA 83771

Observation

Spectrum ID105543953_sp1
Alt nameg1303222-134133
z0.0468
RA, Dec195.8426, -13.6926
MJD61090.71
SNR/Å B/R11.7/18.7
Obs Airmass1.05
SMSS ID105543953
Closest SMSSNone (< 15")
SMSS Mean r6"ap15.2 ± 0.1
2MASS Kext11.7 ± 0.1

AGN Properties

Spectrum TypeSy 1.2
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.040
Power law αν0.40 ± 0.08
log L5100,AGN43.31 ± 0.02
log HβBr/[O III]0.49 ± 0.02
log ML5100/M8.20 ± 0.02
log M/M8.08 ± 0.02
log M/M8.29 ± 0.03
log M[O III]/M8.20 ± 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 Narrow39.87 ± 0.23364 ± 63353 ± 291.27 ± 0.55
Hγ Broad41.20 ± 0.045480 ± 5912196 ± 7126.35 ± 1.26
[O III] 436439.71 ± 0.23340 ± 63144 ± 250.89 ± 0.28
He II Narrow39.30 ± 0.38340 ± 63144 ± 250.41 ± 0.27
He II Broad40.76 ± 0.075461 ± 1392319 ± 5811.68 ± 1.09
Hβ Narrow40.42 ± 0.05364 ± 63353 ± 285.82 ± 0.58
Hβ Broad41.69 ± 0.016269 ± 1232341 ± 31107.47 ± 1.28
[O III] 500741.20 ± 0.01364 ± 63354 ± 2837.94 ± 0.61
He I Narrow39.42 ± 0.22340 ± 63144 ± 250.92 ± 0.27
He I Broad41.10 ± 0.036828 ± 812899 ± 3344.41 ± 1.47
[O I] 630039.82 ± 0.08340 ± 63144 ± 252.74 ± 0.31
Hα Narrow40.97 ± 0.01340 ± 63144 ± 2542.31 ± 0.58
Hα Broad42.27 ± 0.015054 ± 662264 ± 46843.00 ± 2.74
[N II] 658540.52 ± 0.03340 ± 63144 ± 2515.21 ± 0.69
[S II] 671840.28 ± 0.03340 ± 63144 ± 259.23 ± 0.39
[S II] 673240.18 ± 0.04340 ± 63144 ± 257.43 ± 0.39

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 SNR23.69
Hβ Broad SNR7.62
Hγ Broad SNR3.14
AGN frac0.70
Host frac0.30
log L5100,Host42.95
Fe II/Hβ0.19
Fe II/[O III]0.58

Quality flags

spurious_hab/hbb0.0/0
l51002
balmer0
balmer_snr0
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.