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LEDA 90334

Observation

Spectrum ID293179461_sp1
Alt nameg1937330-061305
z0.0104
RA, Dec294.3877, -6.2179
MJD60082.7
SNR/Å B/R5.8/7.6
Obs Airmass1.15
SMSS ID293179461
Closest SMSSNone (< 15")
SMSS Mean r6"ap14.3 ± 0.0
2MASS Kext9.7 ± 0.0

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.249
Power law αν-0.84 ± 0.23
log L5100,AGN43.04 ± 0.03
log HβBr/[O III]-0.10 ± 0.05
log ML5100/M6.76 ± 0.09
log M/M6.56 ± 0.07
log M/M6.66 ± 0.10
log M[O III]/M6.84 ± 0.09

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 Narrow39.90 ± 0.23454 ± 70183 ± 272.99 ± 0.71
Hγ Broad40.65 ± 0.091445 ± 112535 ± 4416.62 ± 1.27
[O III] 436439.48 ± 0.34331 ± 145139 ± 621.43 ± 0.53
He II Narrow39.67 ± 0.32331 ± 145139 ± 622.23 ± 0.45
He II Broad40.11 ± 0.171506 ± 233640 ± 995.52 ± 0.96
Hβ Narrow40.30 ± 0.18454 ± 70183 ± 278.14 ± 0.64
Hβ Broad41.02 ± 0.031363 ± 130492 ± 5343.63 ± 1.06
[O III] 500741.12 ± 0.04454 ± 70183 ± 2759.87 ± 0.71
He I Narrow39.34 ± 0.37331 ± 145139 ± 621.51 ± 0.41
He I Broad40.07 ± 0.141672 ± 127710 ± 536.12 ± 1.15
[O I] 630039.61 ± 0.19331 ± 145139 ± 622.90 ± 0.45
Hα Narrow40.69 ± 0.27331 ± 145139 ± 6233.25 ± 0.91
Hα Broad41.56 ± 0.041446 ± 98485 ± 25214.81 ± 1.41
[N II] 658540.48 ± 0.25331 ± 145139 ± 6220.67 ± 0.69
[S II] 671840.15 ± 0.15331 ± 145139 ± 629.44 ± 0.52
[S II] 673240.11 ± 0.18331 ± 145139 ± 628.63 ± 0.51

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 SNR22.15
Hβ Broad SNR8.77
Hγ Broad SNR3.94
AGN frac0.89
Host frac0.11
log L5100,Host42.14
Fe II/Hβ1.34
Fe II/[O III]1.01

Quality flags

spurious_hab/hbb0.0/0
l51000
balmer0
balmer_snr0
hb_width0
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.