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LEDA 170249

Observation

Spectrum ID105062113_sp1
Alt nameg1327127-245141
z0.0400
RA, Dec201.8031, -24.8613
MJD60353.74
SNR/Å B/R20.0/28.8
Obs Airmass1.01
SMSS ID105062113
Closest SMSSNone (< 15")
SMSS Mean r6"ap16.0 ± 0.0
2MASS Kext11.8 ± 0.1

AGN Properties

Spectrum TypeSy 1.2
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.065
Power law αν-1.19 ± 0.19
log L5100,AGN43.19 ± 0.02
log HβBr/[O III]0.37 ± 0.01
log ML5100/M7.30 ± 0.03
log M/M7.10 ± 0.03
log M/M7.32 ± 0.03
log M[O III]/M7.28 ± 0.03

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 ± 0.08276 ± 63256 ± 292.99 ± 0.39
Hγ Broad40.98 ± 0.022408 ± 136878 ± 3428.01 ± 0.68
[O III] 436439.56 ± 0.15246 ± 63104 ± 251.04 ± 0.21
He II Narrow39.56 ± 0.12246 ± 63104 ± 251.12 ± 0.19
He II Broad41.04 ± 0.0417656 ± 637498 ± 2533.76 ± 1.77
Hβ Narrow40.25 ± 0.04276 ± 63256 ± 295.59 ± 0.39
Hβ Broad41.44 ± 0.012343 ± 501167 ± 2787.30 ± 0.87
[O III] 500741.07 ± 0.01276 ± 63256 ± 2937.83 ± 0.40
He I Narrow39.14 ± 0.23246 ± 63104 ± 250.51 ± 0.17
He I Broad40.68 ± 0.033097 ± 1041315 ± 4317.80 ± 0.62
[O I] 630039.85 ± 0.05246 ± 63104 ± 252.78 ± 0.19
Hα Narrow40.70 ± 0.01246 ± 63104 ± 2520.14 ± 0.29
Hα Broad41.93 ± 0.012087 ± 63908 ± 26340.80 ± 1.10
[N II] 658540.52 ± 0.02246 ± 63104 ± 2513.51 ± 0.26
[S II] 671840.21 ± 0.02246 ± 63104 ± 256.65 ± 0.21
[S II] 673240.11 ± 0.03246 ± 63104 ± 255.35 ± 0.21

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 SNR46.71
Hβ Broad SNR16.43
Hγ Broad SNR7.59
AGN frac0.52
Host frac0.48
log L5100,Host43.16
Fe II/Hβ0.34
Fe II/[O III]0.80

Quality flags

spurious_hab/hbb0.0/0
l51000
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.