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LEDA 132951

Observation

Spectrum ID11026402_sp1
Alt nameg0225363-273048
z0.0641
RA, Dec36.4015, -27.5133
MJD60258.51
SNR/Å B/R13.3/23.7
Obs Airmass1.02
SMSS ID11026402
Closest SMSS9.11'', 2019701720
SMSS Mean r6"ap16.7 ± 0.1
2MASS Kext11.6 ± 0.1

AGN Properties

Spectrum TypeSy 1.2
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.014
Power law αν0.09 ± 0.21
log L5100,AGN43.20 ± 0.03
log HβBr/[O III]0.38 ± 0.04
log ML5100/M7.23 ± 0.04
log M/M6.93 ± 0.03
log M/M7.23 ± 0.05
log M[O III]/M7.19 ± 0.05

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 ± 0.33348 ± 65259 ± 281.44 ± 0.58
Hγ Broad40.65 ± 0.091373 ± 175590 ± 7210.10 ± 1.02
[O III] 436439.27 ± 0.42259 ± 63108 ± 250.43 ± 0.35
He II Narrow39.26 ± 0.39259 ± 63108 ± 250.50 ± 0.41
He II Broad40.44 ± 0.112161 ± 87918 ± 367.45 ± 1.04
Hβ Narrow40.39 ± 0.07348 ± 65259 ± 287.08 ± 0.63
Hβ Broad41.40 ± 0.042172 ± 984085 ± 14573.49 ± 3.38
[O III] 500741.02 ± 0.02348 ± 65259 ± 2832.08 ± 0.69
He I Narrow39.36 ± 0.23259 ± 63108 ± 250.99 ± 0.35
He I Broad40.88 ± 0.0611347 ± 794818 ± 3332.94 ± 2.55
[O I] 630039.55 ± 0.13259 ± 63108 ± 251.78 ± 0.35
Hα Narrow40.70 ± 0.02259 ± 63108 ± 2527.59 ± 0.53
Hα Broad41.78 ± 0.011910 ± 641194 ± 39332.48 ± 3.30
[N II] 658540.67 ± 0.02259 ± 63108 ± 2525.88 ± 0.53
[S II] 671840.05 ± 0.05259 ± 63108 ± 256.44 ± 0.44
[S II] 673240.13 ± 0.04259 ± 63108 ± 257.69 ± 0.46

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 SNR16.46
Hβ Broad SNR4.83
Hγ Broad SNR2.84
AGN frac0.42
Host frac0.58
log L5100,Host43.34
Fe II/Hβ0.42
Fe II/[O III]1.01

Quality flags

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