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LEDA 131234

Observation

Spectrum ID17401582_sp1
Alt nameg0401462-383320
z0.0594
RA, Dec60.4425, -38.5557
MJD59440.68
SNR/Å B/R9.9/22.0
Obs Airmass1.61
SMSS ID17401582
Closest SMSSNone (< 15")
SMSS Mean r6"ap16.8 ± 0.1
2MASS Kext13.2 ± 0.1

AGN Properties

Spectrum TypeSy 1.2
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.005
Power law αν-1.38 ± 0.06
log L5100,AGN43.07 ± 0.02
log HβBr/[O III]0.51 ± 0.05
log ML5100/M7.11 ± 0.14
log M/M6.81 ± 0.04
log M/M7.05 ± 0.14
log M[O III]/M6.93 ± 0.15

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 Narrow39.80 ± 0.21249 ± 63263 ± 342.46 ± 0.89
Hγ Broad40.28 ± 0.182145 ± 634971 ± 1296.57 ± 1.79
[O III] 436439.55 ± 0.22215 ± 6391 ± 251.40 ± 0.45
He II Narrow39.61 ± 0.17215 ± 6391 ± 251.68 ± 0.41
He II Broad40.82 ± 0.078412 ± 1463572 ± 6126.88 ± 2.62
Hβ Narrow40.42 ± 0.05249 ± 63263 ± 3411.03 ± 0.80
Hβ Broad41.13 ± 0.032011 ± 3082567 ± 8056.75 ± 2.57
[O III] 500740.62 ± 0.03249 ± 63263 ± 3417.83 ± 0.81
He I Narrow
He I Broad40.17 ± 0.072149 ± 123913 ± 526.79 ± 0.72
[O I] 630039.46 ± 0.10215 ± 6391 ± 251.44 ± 0.20
Hα Narrow40.82 ± 0.01215 ± 6391 ± 2533.41 ± 0.29
Hα Broad41.39 ± 0.012184 ± 74909 ± 28123.91 ± 1.02
[N II] 658540.44 ± 0.02215 ± 6391 ± 2514.16 ± 0.26
[S II] 671840.07 ± 0.03215 ± 6391 ± 256.00 ± 0.23
[S II] 673239.99 ± 0.03215 ± 6391 ± 254.99 ± 0.23

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 SNR8.94
Hβ Broad SNR3.71
Hγ Broad SNR1.05
AGN frac0.49
Host frac0.51
log L5100,Host43.09
Fe II/Hβ0.43
Fe II/[O III]1.40

Quality flags

spurious_hab/hbb0.0/0
l51001
balmer0
balmer_snr1
hb_width2
balmer_width1

Hα mass estimates from Cho+2023. Remaining mass estimates from R–L relations in Wang & Woo 2024 and zero-points from Amrutha+2026.