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LEDA 1014434

Observation

Spectrum ID13037273_sp1
Alt nameg0040528-074209
z0.0546
RA, Dec10.2200, -7.7024
MJD59079.76
SNR/Å B/R19.7/37.1
Obs Airmass1.15
SMSS ID13037273
Closest SMSSNone (< 15")
SMSS Mean r6"ap15.7 ± 0.0
2MASS Kext11.7 ± 0.1

AGN Properties

Spectrum TypeSy 1.2
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.039
Power law αν0.43 ± 0.06
log L5100,AGN43.33 ± 0.01
log HβBr/[O III]0.45 ± 0.01
log ML5100/M8.17 ± 0.02
log M/M7.94 ± 0.01
log M/M8.22 ± 0.02
log M[O III]/M8.16 ± 0.02

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 Narrow39.72 ± 0.24402 ± 63285 ± 330.84 ± 0.43
Hγ Broad41.22 ± 0.034935 ± 2491895 ± 4226.15 ± 0.95
[O III] 436439.72 ± 0.21390 ± 63165 ± 250.86 ± 0.25
He II Narrow39.76 ± 0.16390 ± 63165 ± 251.11 ± 0.26
He II Broad41.12 ± 0.048581 ± 1513644 ± 6325.48 ± 1.27
Hβ Narrow40.56 ± 0.03402 ± 63286 ± 337.73 ± 0.52
Hβ Broad41.63 ± 0.015988 ± 821975 ± 2989.91 ± 0.95
[O III] 500741.18 ± 0.01402 ± 63286 ± 3334.43 ± 0.57
He I Narrow39.51 ± 0.18390 ± 63165 ± 251.08 ± 0.25
He I Broad41.09 ± 0.025592 ± 912375 ± 3740.80 ± 1.03
[O I] 630040.00 ± 0.05390 ± 63165 ± 253.93 ± 0.30
Hα Narrow41.20 ± 0.01390 ± 63165 ± 2568.77 ± 0.46
Hα Broad42.12 ± 0.014787 ± 731855 ± 25580.61 ± 1.42
[N II] 658540.86 ± 0.01390 ± 63165 ± 2531.87 ± 0.43
[S II] 671840.41 ± 0.02390 ± 63165 ± 2511.93 ± 0.37
[S II] 673240.37 ± 0.02390 ± 63165 ± 2510.97 ± 0.38

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 SNR21.94
Hβ Broad SNR8.38
Hγ Broad SNR4.06
AGN frac0.44
Host frac0.56
log L5100,Host43.43
Fe II/Hβ0.42
Fe II/[O III]1.18

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.