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LEDA 3094039

Observation

Spectrum ID11934338_sp1
Alt nameg0023554-180251
z0.0533
RA, Dec5.9807, -18.0474
MJD60259.46
SNR/Å B/R12.0/20.9
Obs Airmass1.03
SMSS ID11934338
Closest SMSSNone (< 15")
SMSS Mean r6"ap16.8 ± 0.1
2MASS Kext13.4 ± 0.2

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.020
Power law αν-0.18 ± 0.19
log L5100,AGN43.06 ± 0.04
log HβBr/[O III]-0.25 ± 0.03
log ML5100/M7.78 ± 0.06
log M/M7.13 ± 0.03
log M/M7.72 ± 0.07
log M[O III]/M7.97 ± 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 Narrow40.02 ± 0.09228 ± 62208 ± 263.44 ± 0.56
Hγ Broad40.58 ± 0.093087 ± 5581239 ± 12111.90 ± 1.33
[O III] 436439.85 ± 0.09196 ± 6283 ± 252.33 ± 0.30
He II Narrow39.67 ± 0.11196 ± 6283 ± 251.75 ± 0.30
He II Broad40.72 ± 0.077523 ± 4053195 ± 17219.39 ± 1.78
Hβ Narrow40.52 ± 0.02228 ± 62208 ± 2613.49 ± 0.56
Hβ Broad41.12 ± 0.034374 ± 2641814 ± 9552.70 ± 1.69
[O III] 500741.37 ± 0.01228 ± 62208 ± 2699.71 ± 0.74
He I Narrow39.05 ± 0.22196 ± 6283 ± 250.64 ± 0.23
He I Broad40.44 ± 0.063846 ± 2511633 ± 10615.99 ± 1.20
[O I] 630039.94 ± 0.03196 ± 6283 ± 255.64 ± 0.26
Hα Narrow40.89 ± 0.01196 ± 6283 ± 2554.49 ± 0.42
Hα Broad41.62 ± 0.012700 ± 701379 ± 63288.40 ± 2.64
[N II] 658540.51 ± 0.01196 ± 6283 ± 2522.76 ± 0.37
[S II] 671840.27 ± 0.02196 ± 6283 ± 2513.58 ± 0.33
[S II] 673240.20 ± 0.02196 ± 6283 ± 2511.66 ± 0.32

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 SNR12.65
Hβ Broad SNR3.65
Hγ Broad SNR1.80
AGN frac0.51
Host frac0.49
log L5100,Host43.04
Fe II/Hβ0.53
Fe II/[O III]0.29

Quality flags

spurious_hab/hbb0.0/0
l51000
balmer0
balmer_snr1
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.