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LEDA 991676

Observation

Spectrum ID109988713_sp1
Alt nameg1423502-092318
z0.0682
RA, Dec215.9594, -9.3882
MJD60018.69
SNR/Å B/R7.7/14.9
Obs Airmass1.08
SMSS ID109988713
Closest SMSSNone (< 15")
SMSS Mean r6"ap17.0 ± 0.1
2MASS Kext13.6 ± 0.2

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.053
Power law αν0.06 ± 0.21
log L5100,AGN43.22 ± 0.03
log HβBr/[O III]0.16 ± 0.04
log ML5100/M7.19 ± 0.07
log M/M6.70 ± 0.04
log M/M7.16 ± 0.07
log M[O III]/M7.23 ± 0.07

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 Narrow40.18 ± 0.12266 ± 63310 ± 323.37 ± 0.97
Hγ Broad40.71 ± 0.102486 ± 311914 ± 8710.77 ± 1.40
[O III] 436440.03 ± 0.13256 ± 63108 ± 252.39 ± 0.43
He II Narrow39.60 ± 0.26256 ± 63108 ± 251.03 ± 0.42
He II Broad40.85 ± 0.073879 ± 2251647 ± 9518.51 ± 1.72
Hβ Narrow40.58 ± 0.05266 ± 63310 ± 3210.69 ± 1.02
Hβ Broad41.35 ± 0.032044 ± 1561707 ± 11462.67 ± 2.54
[O III] 500741.19 ± 0.02266 ± 63310 ± 3246.27 ± 1.13
He I Narrow39.20 ± 0.31256 ± 63108 ± 250.65 ± 0.30
He I Broad40.39 ± 0.072143 ± 169910 ± 7110.30 ± 0.98
[O I] 630039.63 ± 0.11256 ± 63108 ± 252.02 ± 0.34
Hα Narrow41.02 ± 0.01256 ± 63108 ± 2554.47 ± 0.50
Hα Broad41.75 ± 0.011496 ± 65720 ± 25292.05 ± 1.52
[N II] 658540.56 ± 0.02256 ± 63108 ± 2518.86 ± 0.49
[S II] 671840.30 ± 0.03256 ± 63108 ± 2510.74 ± 0.53
[S II] 673240.10 ± 0.05256 ± 63108 ± 256.92 ± 0.54

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 SNR17.92
Hβ Broad SNR5.53
Hγ Broad SNR1.77
AGN frac0.63
Host frac0.37
log L5100,Host42.99
Fe II/Hβ0.39
Fe II/[O III]0.56

Quality flags

spurious_hab/hbb0.0/0
l51000
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.