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LEDA 50427

Observation

Spectrum ID101980617_sp1
Alt nameg1408068-302354
z0.0237
RA, Dec212.0283, -30.3983
MJD60077.52
SNR/Å B/R15.0/23.1
Obs Airmass1.00
SMSS ID101980617
Closest SMSSNone (< 15")
SMSS Mean r6"ap15.4 ± 0.1
2MASS Kext12.4 ± 0.1

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.051
Power law αν-0.64 ± 0.08
log L5100,AGN43.03 ± 0.01
log HβBr/[O III]0.20 ± 0.01
log ML5100/M7.44 ± 0.03
log M/M7.12 ± 0.02
log M/M7.49 ± 0.03
log M[O III]/M7.54 ± 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 Narrow39.63 ± 0.11298 ± 63204 ± 261.64 ± 0.33
Hγ Broad40.87 ± 0.022912 ± 1261075 ± 4128.14 ± 0.66
[O III] 436439.88 ± 0.05281 ± 63117 ± 252.95 ± 0.20
He II Narrow39.57 ± 0.07281 ± 63117 ± 251.61 ± 0.18
He II Broad40.88 ± 0.025490 ± 1492331 ± 6232.66 ± 0.78
Hβ Narrow40.09 ± 0.03298 ± 63204 ± 265.54 ± 0.32
Hβ Broad41.35 ± 0.013000 ± 641476 ± 5499.75 ± 0.91
[O III] 500741.14 ± 0.01298 ± 63204 ± 2665.46 ± 0.34
He I Narrow38.70 ± 0.30281 ± 63117 ± 250.29 ± 0.13
He I Broad40.36 ± 0.032736 ± 1371162 ± 5813.25 ± 0.51
[O I] 630039.54 ± 0.04281 ± 63117 ± 252.23 ± 0.15
Hα Narrow40.52 ± 0.01281 ± 63117 ± 2522.66 ± 0.28
Hα Broad41.82 ± 0.012324 ± 641139 ± 25443.45 ± 0.84
[N II] 658539.74 ± 0.05281 ± 63117 ± 253.78 ± 0.23
[S II] 671839.69 ± 0.04281 ± 63117 ± 253.43 ± 0.19
[S II] 673239.53 ± 0.05281 ± 63117 ± 252.40 ± 0.18

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 SNR51.36
Hβ Broad SNR18.06
Hγ Broad SNR8.26
AGN frac0.81
Host frac0.19
log L5100,Host42.39
Fe II/Hβ0.13
Fe II/[O III]0.20

Quality flags

spurious_hab/hbb0.0/0
l51000
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.