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LEDA 225607

Observation

Spectrum ID408665904_sp1
Alt nameg1514420-812338
z0.0682
RA, Dec228.6750, -81.3939
MJD59015.55
SNR/Å B/R16.9/26.9
Obs Airmass1.58
SMSS ID408665904
Closest SMSS14.08'', 408665905
SMSS Mean r6"ap16.0 ± 0.1
2MASS Kext12.0 ± 0.1

AGN Properties

Spectrum TypeSy 1.2
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.234
Power law αν0.16 ± 0.15
log L5100,AGN44.08 ± 0.03
log HβBr/[O III]0.34 ± 0.06
log ML5100/M8.99 ± 0.13
log M/M8.89 ± 0.10
log M/M9.09 ± 0.13
log M[O III]/M9.11 ± 0.13

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 Narrow40.40 ± 0.28407 ± 69308 ± 500.75 ± 0.29
Hγ Broad41.42 ± 0.302477 ± 15311211 ± 8927.88 ± 0.58
[O III] 436440.67 ± 0.13361 ± 69153 ± 281.39 ± 0.17
He II Narrow40.26 ± 0.23361 ± 69153 ± 280.65 ± 0.17
He II Broad40.97 ± 0.172773 ± 9071178 ± 3853.43 ± 0.49
Hβ Narrow40.95 ± 0.09407 ± 69309 ± 503.38 ± 0.33
Hβ Broad42.46 ± 0.0610539 ± 16854241 ± 635110.44 ± 1.18
[O III] 500742.12 ± 0.01407 ± 69309 ± 5053.92 ± 0.39
He I Narrow39.91 ± 0.29361 ± 69153 ± 280.47 ± 0.16
He I Broad40.81 ± 0.331399 ± 628594 ± 2663.67 ± 0.36
[O I] 630040.77 ± 0.06361 ± 69153 ± 283.93 ± 0.19
Hα Narrow41.52 ± 0.06361 ± 69153 ± 2823.16 ± 0.29
Hα Broad42.89 ± 0.018344 ± 8443322 ± 97549.51 ± 1.42
[N II] 658541.52 ± 0.08361 ± 69153 ± 2823.19 ± 0.30
[S II] 671840.83 ± 0.05361 ± 69153 ± 285.16 ± 0.26
[S II] 673240.88 ± 0.06361 ± 69153 ± 285.75 ± 0.27

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 SNR18.10
Hβ Broad SNR7.45
Hγ Broad SNR3.03
AGN frac0.82
Host frac0.18
log L5100,Host43.42
Fe II/Hβ0.27
Fe II/[O III]0.59

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.