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LEDA 14727

Observation

Spectrum ID24422052_sp1
Alt nameg0414527-075540
z0.0381
RA, Dec63.7194, -7.9277
MJD60266.57
SNR/Å B/R5.9/9.9
Obs Airmass1.11
SMSS ID24422052
Closest SMSSNone (< 15")
SMSS Mean r6"ap14.6 ± 0.1
2MASS Kextnan ± nan

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.072
Power law αν0.18 ± 0.21
log L5100,AGN43.86 ± 0.02
log HβBr/[O III]-0.41 ± 0.03
log ML5100/M8.10 ± 0.07
log M/M7.93 ± 0.09
log M/M8.18 ± 0.07
log M[O III]/M8.56 ± 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 Narrow41.09 ± 0.08253 ± 63149 ± 295.92 ± 0.69
Hγ Broad41.59 ± 0.082166 ± 506889 ± 13118.44 ± 1.47
[O III] 436441.02 ± 0.07240 ± 63100 ± 255.43 ± 0.47
He II Narrow40.80 ± 0.10240 ± 63100 ± 253.78 ± 0.42
He II Broad41.09 ± 0.131685 ± 214715 ± 907.23 ± 1.08
Hβ Narrow41.50 ± 0.03253 ± 63149 ± 2920.15 ± 0.77
Hβ Broad42.20 ± 0.034246 ± 3341515 ± 13898.17 ± 1.91
[O III] 500742.61 ± 0.01253 ± 63149 ± 29278.01 ± 1.33
He I Narrow40.32 ± 0.15240 ± 63100 ± 252.09 ± 0.38
He I Broad41.16 ± 0.092700 ± 3151146 ± 13313.24 ± 1.22
[O I] 630040.76 ± 0.06240 ± 63100 ± 256.57 ± 0.45
Hα Narrow41.99 ± 0.03240 ± 63100 ± 25121.56 ± 1.23
Hα Broad42.87 ± 0.012802 ± 2891513 ± 79924.45 ± 3.18
[N II] 658540.80 ± 0.18240 ± 63100 ± 257.75 ± 0.87
[S II] 671841.03 ± 0.04240 ± 63100 ± 2514.06 ± 0.56
[S II] 673240.88 ± 0.05240 ± 63100 ± 2510.03 ± 0.54

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 SNR25.09
Hβ Broad SNR5.95
Hγ Broad SNR3.01
AGN frac0.79
Host frac0.20
log L5100,Host43.27
Fe II/Hβ0.27
Fe II/[O III]0.10

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.