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LEDA 163530

Observation

Spectrum ID3979095_sp1
Alt nameg2158596-175245
z0.0938
RA, Dec329.7485, -17.8793
MJD60091.77
SNR/Å B/R14.2/20.6
Obs Airmass1.07
SMSS ID3979095
Closest SMSS6.31'', 2006997536
SMSS Mean r6"ap15.8 ± 0.2
2MASS Kext11.7 ± 0.1

AGN Properties

Spectrum TypeSy 1.0
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.039
Power law αν0.48 ± 0.01
log L5100,AGN43.87 ± 0.01
log HβBr/[O III]1.05 ± 0.03
log ML5100/M8.89 ± 0.02
log M/M8.61 ± 0.03
log M/M9.02 ± 0.02
log M[O III]/M8.69 ± 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 Narrow40.13 ± 0.45770 ± 67322 ± 250.62 ± 0.35
Hγ Broad40.87 ± 0.171873 ± 130705 ± 502.83 ± 0.60
[O III] 436440.73 ± 0.10548 ± 63232 ± 252.51 ± 0.34
He II Narrow39.95 ± 0.43548 ± 63232 ± 250.50 ± 0.33
He II Broad40.49 ± 0.302157 ± 64916 ± 261.72 ± 0.66
Hβ Narrow39.98 ± 0.46770 ± 67322 ± 250.59 ± 0.48
Hβ Broad42.34 ± 0.0110490 ± 2323889 ± 25134.52 ± 2.16
[O III] 500741.29 ± 0.03770 ± 67322 ± 2512.73 ± 0.51
He I Narrow39.74 ± 0.41548 ± 63232 ± 250.53 ± 0.36
He I Broad41.47 ± 0.046882 ± 632922 ± 2528.89 ± 1.43
[O I] 630040.15 ± 0.22548 ± 63232 ± 251.66 ± 0.51
Hα Narrow41.37 ± 0.02548 ± 63232 ± 2530.31 ± 0.67
Hα Broad42.67 ± 0.017047 ± 782482 ± 25604.56 ± 2.28
[N II] 658541.44 ± 0.02548 ± 63232 ± 2536.20 ± 0.68
[S II] 671840.68 ± 0.08548 ± 63232 ± 256.61 ± 0.68
[S II] 673240.53 ± 0.10548 ± 63232 ± 254.64 ± 0.68

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 SNR13.89
Hβ Broad SNR5.75
Hγ Broad SNR1.23
AGN frac0.64
Host frac0.36
log L5100,Host43.61
Fe II/Hβ0.50
Fe II/[O III]5.64

Quality flags

spurious_hab/hbb0.0/0
l51002
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.